This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn
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 20.0788* 00 35 58.92 +65 01 35.6 11.1 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
TOI 1568.01,2461119.5788,11.09,0.05,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
TOI 1568.01 20260320.0788 11.09CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:58.92 +65:01:35.6 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 10.79 00:32:56.21 +65:13:04.3
120.99316 2.41578 galactic Cas Second-epoch detections are separated by 2.1" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527166076923369600 | 00:32:57.49 +65:13:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1966UppAn...5d...1O [O66] 8:1176
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 20.0788* 00 32 56.21 +65 13 04.3 10.8 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
Gaia DR3 527166076923369600,2461119.5788,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527166076923369600 20260320.0788 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:56.21 +65:13:04.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 46 12.54 +57 13 12.6 10.4 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
V1051 Cas,2461119.5788,10.40,0.05,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
V1051 Cas 20260320.0788 10.40CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:12.54 +57:13:12.6 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 02 38 00.96 +63 01 46.6 11.1 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
V0488 Cas,2461119.5788,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0488 Cas 20260320.0788 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:38:00.96 +63:01:46.6 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 46 54.08 +56 40 16.0 11.1 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
GW Cas,2461119.5788,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GW Cas 20260320.0788 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:54.08 +56:40:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 45 28.44 +57 19 14.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0045275+571904,2461119.5788,11.37,0.05,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 J0045275+571904 20260320.0788 11.37CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:28.44 +57:19:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 46 55.79 +63 56 06.7 10.9 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
V0661 Cas,2461119.5788,10.94,0.05,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
V0661 Cas 20260320.0788 10.94CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:55.79 +63:56:06.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 28 36.98 +62 16 38.8 10.8 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
V0390 Cas,2461119.5788,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0390 Cas 20260320.0788 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:28:36.98 +62:16:38.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 54 54.27 +58 33 50.7 8.7 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
W Cas,2461119.5788,8.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
W Cas 20260320.0788 8.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:54:54.27 +58:33:50.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 23 00.84 +64 39 24.5 10.7 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
V0900 Cas,2461119.5788,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0900 Cas 20260320.0788 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:23:00.84 +64:39:24.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 02 30 27.23 +62 31 46.5 10.3 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
V0647 Cas,2461119.5788,10.30,0.05,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
V0647 Cas 20260320.0788 10.30CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:30:27.23 +62:31:46.5 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 13.00 00:39:24.46 +64:30:15.8
121.63728 1.66289 galactic Cas Second-epoch detections are separated by 2.7" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ZTF J003928.60+642938.3 | 00:39:28.60 +64:29:38.4 (Gaia DR3) | SR (local) | 2458286.78640 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 39 24.46 +64 30 15.8 13.0 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
ZTF J003928.60+642938.3,2461119.5788,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J003928.60+642938.3 20260320.0788 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:24.46 +64:30:15.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.88 00:37:33.55 +62:02:14.3
121.30561 -0.79061 galactic Cas Second-epoch detections are separated by 3.0" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 430657577666659968 | 00:37:34.48 +62:02:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 37 33.55 +62 02 14.3 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
Gaia DR3 430657577666659968,2461119.5788,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430657577666659968 20260320.0788 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:33.55 +62:02:14.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 39 37.31 +66 00 20.5 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
Gaia DR3 527647113255714432,2461119.5788,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527647113255714432 20260320.0788 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:37.31 +66:00:20.5 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.85 00:49:24.50 +58:00:18.0
122.66211 -4.86569 galactic Cas Second-epoch detections are separated by 3.9" and 0.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 425066389239117184 | 00:49:23.50 +58:00:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 49 24.50 +58 00 18.0 12.8 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
Gaia DR3 425066389239117184,2461119.5788,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425066389239117184 20260320.0788 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:49:24.50 +58:00:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.80 00:38:07.46 +61:40:25.8
121.35299 -1.15709 galactic Cas Second-epoch detections are separated by 5.2" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 427269707464641408 | 00:38:06.74 +61:40:29.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 38 07.46 +61 40 25.8 12.8 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
Gaia DR3 427269707464641408,2461119.5788,12.80,0.05,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
Gaia DR3 427269707464641408 20260320.0788 12.80CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:07.46 +61:40:25.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 42 46.79 +65 05 55.8 12.7 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
Gaia DR3 524484505495584000,2461119.5788,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524484505495584000 20260320.0788 12.74CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:46.79 +65:05:55.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.88 00:35:09.74 +66:10:21.1
121.28649 3.35279 galactic Cas Second-epoch detections are separated by 1.5" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527617353421164928 | 00:35:07.90 +66:10:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 35 09.74 +66 10 21.1 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
Gaia DR3 527617353421164928,2461119.5788,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527617353421164928 20260320.0788 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:09.74 +66:10:21.1 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 36 44.04 +62 48 52.5 12.8 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
Gaia DR3 430708876756634368,2461119.5788,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430708876756634368 20260320.0788 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:44.04 +62:48:52.5 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.64 00:37:26.01 +64:50:45.9
121.44361 2.01481 galactic Cas Second-epoch detections are separated by 8.0" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527096120493379840 | 00:37:27.18 +64:50:45.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 37 26.01 +64 50 45.9 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
Gaia DR3 527096120493379840,2461119.5788,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527096120493379840 20260320.0788 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:26.01 +64:50:45.9 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.54 00:40:27.59 +64:33:43.2
121.75289 1.71539 galactic Cas Second-epoch detections are separated by 3.7" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527072858950834176 | 00:40:26.76 +64:33:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 40 27.59 +64 33 43.2 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
Gaia DR3 527072858950834176,2461119.5788,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527072858950834176 20260320.0788 12.54CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:27.59 +64:33:43.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.61 00:37:18.58 +64:11:56.4
121.39495 1.36942 galactic Cas Second-epoch detections are separated by 5.5" and 0.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 526979056864976768 | 00:37:16.53 +64:11:55.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 37 18.58 +64 11 56.4 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
Gaia DR3 526979056864976768,2461119.5788,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 526979056864976768 20260320.0788 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:18.58 +64:11:56.4 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.64 00:33:03.73 +64:29:55.5
120.95494 1.69756 galactic Cas Second-epoch detections are separated by 4.5" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527045955276691200 | 00:33:00.91 +64:29:56.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 33 03.73 +64 29 55.5 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
Gaia DR3 527045955276691200,2461119.5788,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527045955276691200 20260320.0788 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:03.73 +64:29:55.5 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.67 00:35:10.32 +65:28:35.7
121.24342 2.65818 galactic Cas Second-epoch detections are separated by 4.4" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527184871699511680 | 00:35:08.78 +65:28:36.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 35 10.32 +65 28 35.7 12.7 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
Gaia DR3 527184871699511680,2461119.5788,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527184871699511680 20260320.0788 12.67CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:10.32 +65:28:35.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.59 00:37:14.10 +64:34:40.8
121.40774 1.74829 galactic Cas Second-epoch detections are separated by 5.8" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527084781779849600 | 00:37:11.57 +64:34:40.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +64 28
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 20.0788* 00 37 14.10 +64 34 40.8 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
Gaia DR3 527084781779849600,2461119.5788,12.59,0.05,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
Gaia DR3 527084781779849600 20260320.0788 12.59CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:14.10 +64:34:40.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.37 00:36:14.79 +64:20:13.2
121.28756 1.51376 galactic Cas Second-epoch detections are separated by 2.0" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 526982149241288448 | 00:36:13.20 +64:20:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 36 14.79 +64 20 13.2 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
Gaia DR3 526982149241288448,2461119.5788,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 526982149241288448 20260320.0788 12.37CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:14.79 +64:20:13.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 36 56.00 +63 24 13.7 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
Gaia DR3 430852809700054272,2461119.5788,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430852809700054272 20260320.0788 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:56.00 +63:24:13.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.46 00:30:22.65 +65:18:31.4
120.73295 2.52693 galactic Cas Second-epoch detections are separated by 2.8" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527357391940894208 | 00:30:25.11 +65:18:31.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 30 22.65 +65 18 31.4 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
Gaia DR3 527357391940894208,2461119.5788,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527357391940894208 20260320.0788 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:22.65 +65:18:31.4 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.38 00:37:07.51 +62:10:06.0
121.26209 -0.65700 galactic Cas Second-epoch detections are separated by 1.6" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 430660841832078080 | 00:37:08.98 +62:10:09.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 37 07.51 +62 10 06.0 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
Large-amplitude variable Gaia DR2 430660841832078080,2461119.5788,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 430660841832078080 20260320.0788 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:07.51 +62:10:06.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 37 12.58 +65 18 00.7 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
Gaia DR3 527179271062236288,2461119.5788,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527179271062236288 20260320.0788 12.43CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:12.58 +65:18:00.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.44 00:41:51.84 +63:45:47.7
121.87392 0.91117 galactic Cas Second-epoch detections are separated by 0.4" and 1.2 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 | Gaia DR3 523949691870346240 | 00:41:50.53 +63:45:46.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 41 51.84 +63 45 47.7 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
Gaia DR3 523949691870346240,2461119.5788,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523949691870346240 20260320.0788 12.44CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:51.84 +63:45:47.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.41 00:40:58.96 +64:53:57.0
121.82271 2.04994 galactic Cas Second-epoch detections are separated by 3.8" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527107871524805120 | 00:41:00.29 +64:54:00.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 40 58.96 +64 53 57.0 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
Gaia DR3 527107871524805120,2461119.5788,12.41,0.05,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
Gaia DR3 527107871524805120 20260320.0788 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:58.96 +64:53:57.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.23 00:30:16.03 +65:30:32.7
120.73794 2.72756 galactic Cas Second-epoch detections are separated by 1.4" and 1.2 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 | Gaia DR3 527384261256222336 | 00:30:14.95 +65:30:33.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 30 16.03 +65 30 32.7 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
Gaia DR3 527384261256222336,2461119.5788,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527384261256222336 20260320.0788 12.23CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:16.03 +65:30:32.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.28 00:37:50.92 +64:51:50.1
121.48863 2.03026 galactic Cas Second-epoch detections are separated by 3.0" and 0.9 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 | Large-amplitude variable Gaia DR2 527095845615883264 | 00:37:49.91 +64:51:47.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 37 50.92 +64 51 50.1 12.3 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
Large-amplitude variable Gaia DR2 527095845615883264,2461119.5788,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 527095845615883264 20260320.0788 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:50.92 +64:51:50.1 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.24 00:32:53.14 +64:03:49.7
120.90467 1.26511 galactic Cas Second-epoch detections are separated by 6.5" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527009430866811008 | 00:32:50.24 +64:03:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 32 53.14 +64 03 49.7 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
Gaia DR3 527009430866811008,2461119.5788,12.24,0.05,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
Gaia DR3 527009430866811008 20260320.0788 12.24CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:53.14 +64:03:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.24 00:40:36.68 +63:51:02.8
121.73924 1.00410 galactic Cas Second-epoch detections are separated by 0.7" and 1.2 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 | Gaia DR3 526956482517062912 | 00:40:35.14 +63:51:01.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 40 36.68 +63 51 02.8 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
Gaia DR3 526956482517062912,2461119.5788,12.24,0.05,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
Gaia DR3 526956482517062912 20260320.0788 12.24CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:36.68 +63:51:02.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 38 49.11 +61 56 26.2 12.1 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
Gaia DR3 427653505740015488,2461119.5788,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427653505740015488 20260320.0788 12.09CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:49.11 +61:56:26.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 42 15.95 +60 40 52.7 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
CzeV2987,2461119.5788,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CzeV2987 20260320.0788 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:15.95 +60:40:52.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.10 00:31:03.31 +65:40:09.8
120.83213 2.88078 galactic Cas Second-epoch detections are separated by 2.0" and 1.2 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 | Gaia DR3 527391992197311104 | 00:31:01.64 +65:40:11.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 31 03.31 +65 40 09.8 12.1 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
Gaia DR3 527391992197311104,2461119.5788,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527391992197311104 20260320.0788 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:03.31 +65:40:09.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.96 00:43:02.96 +63:44:54.8
122.00438 0.89192 galactic Cas Second-epoch detections are separated by 7.4" and 0.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 523938563619643392 | 00:43:01.67 +63:44:53.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 43 02.96 +63 44 54.8 12.0 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
Gaia DR3 523938563619643392,2461119.5788,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523938563619643392 20260320.0788 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:02.96 +63:44:54.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.10 00:38:28.77 +62:18:21.9
121.42688 -0.52779 galactic Cas Second-epoch detections are separated by 2.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 427666012684561280 | 00:38:29.99 +62:18:24.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 38 28.77 +62 18 21.9 12.1 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
Gaia DR3 427666012684561280,2461119.5788,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427666012684561280 20260320.0788 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:28.77 +62:18:21.9 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.04 00:40:50.30 +65:22:29.8
121.82701 2.52594 galactic Cas Second-epoch detections are separated by 3.7" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527499194582153472 | 00:40:49.39 +65:22:27.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.733+/-0.090 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 40 50.30 +65 22 29.8 12.0 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
Gaia DR3 527499194582153472,2461119.5788,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527499194582153472 20260320.0788 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:50.30 +65:22:29.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 02 33 32.98 +57 32 55.4 12.2 U Per 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
Gaia DR3 458024662599409664,2461119.5788,12.24,0.05,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
Gaia DR3 458024662599409664 20260320.0788 12.24CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:33:32.98 +57:32:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 41 10.21 +60 52 06.8 12.0 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
CzeV4228,2461119.5788,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CzeV4228 20260320.0788 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:10.21 +60:52:06.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.94 00:35:51.26 +62:51:44.3
121.15596 0.04431 galactic Cas Second-epoch detections are separated by 2.8" and 0.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 430721654283188992 | 00:35:50.16 +62:51:41.0 (Gaia DR3) | S (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 35 51.26 +62 51 44.3 11.9 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
Gaia DR3 430721654283188992,2461119.5788,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430721654283188992 20260320.0788 11.94CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:51.26 +62:51:44.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.93 00:39:40.03 +65:15:11.8
121.69944 2.40970 galactic Cas Second-epoch detections are separated by 2.9" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527502699275540224 | 00:39:41.30 +65:15:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 39 40.03 +65 15 11.8 11.9 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
Gaia DR3 527502699275540224,2461119.5788,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527502699275540224 20260320.0788 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:40.03 +65:15:11.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 41 16.70 +65 57 56.0 11.8 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
Gaia DR3 527643127527266432,2461119.5788,11.80,0.05,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
Gaia DR3 527643127527266432 20260320.0788 11.80CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:16.70 +65:57:56.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.82 00:33:56.56 +64:29:16.2
121.04878 1.68007 galactic Cas Second-epoch detections are separated by 3.7" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527034784058010880 | 00:33:53.33 +64:29:20.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 33 56.56 +64 29 16.2 11.8 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
Gaia DR3 527034784058010880,2461119.5788,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 527034784058010880 20260320.0788 11.82CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:56.56 +64:29:16.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.74 00:35:38.90 +62:57:03.6
121.13795 0.13426 galactic Cas Second-epoch detections are separated by 1.2" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 430722517572634624 | 00:35:37.83 +62:57:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 35 38.90 +62 57 03.6 11.7 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
Gaia DR3 430722517572634624,2461119.5788,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430722517572634624 20260320.0788 11.74CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:38.90 +62:57:03.6 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.82 00:43:21.34 +64:17:02.3
122.05505 1.42598 galactic Cas Second-epoch detections are separated by 0.5" and 1.2 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 | Gaia DR3 524062945872931840 | 00:43:19.35 +64:17:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB 1954BOTT....1j..28M [M54] 91
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 20.0788* 00 43 21.34 +64 17 02.3 11.8 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
Gaia DR3 524062945872931840,2461119.5788,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524062945872931840 20260320.0788 11.82CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:21.34 +64:17:02.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.64 00:36:07.37 +63:18:57.4
121.21349 0.49531 galactic Cas Second-epoch detections are separated by 3.4" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 430828036327581184 | 00:36:06.16 +63:18:55.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 36 07.37 +63 18 57.4 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
Large-amplitude variable Gaia DR2 430828036327581184,2461119.5788,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 430828036327581184 20260320.0788 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:07.37 +63:18:57.4 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.61 00:36:58.76 +63:27:39.3
121.31762 0.63450 galactic Cas Second-epoch detections are separated by 2.1" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 430853359448212992 | 00:36:59.67 +63:27:41.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 36 58.76 +63 27 39.3 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
Gaia DR3 430853359448212992,2461119.5788,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430853359448212992 20260320.0788 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:58.76 +63:27:39.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.51 00:32:19.67 +64:34:53.0
120.88221 1.78572 galactic Cas Second-epoch detections are separated by 5.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 527049494329894272 | 00:32:22.23 +64:34:54.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 32 19.67 +64 34 53.0 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
Gaia DR3 527049494329894272,2461119.5788,11.51,0.05,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
Gaia DR3 527049494329894272 20260320.0788 11.51CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:19.67 +64:34:53.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 39 32.86 +63 41 01.9 11.3 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
Gaia DR3 526925215154528256,2461119.5788,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 526925215154528256 20260320.0788 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:32.86 +63:41:01.9 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.55 00:39:46.41 +63:06:41.6
121.61353 0.26967 galactic Cas Second-epoch detections are separated by 1.8" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 427830698911276032 | 00:39:45.60 +63:06:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 39 46.41 +63 06 41.6 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
Gaia DR3 427830698911276032,2461119.5788,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427830698911276032 20260320.0788 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:46.41 +63:06:41.6 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.31 00:41:55.23 +59:49:28.4
121.73452 -3.02506 galactic Cas Second-epoch detections are separated by 0.9" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 425502002002287232 | 00:41:54.40 +59:49:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 41 55.23 +59 49 28.4 11.3 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
Gaia DR3 425502002002287232,2461119.5788,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425502002002287232 20260320.0788 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:55.23 +59:49:28.4 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 10.88 00:42:50.41 +59:11:09.9
121.82880 -3.66725 galactic Cas Second-epoch detections are separated by 2.3" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 425458674371600768 | 00:42:51.16 +59:11:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 42 50.41 +59 11 09.9 10.9 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
Gaia DR3 425458674371600768,2461119.5788,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425458674371600768 20260320.0788 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:50.41 +59:11:09.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 9.38 00:45:52.94 +58:02:26.8
122.19419 -4.82301 galactic Cas Second-epoch detections are separated by 0.5" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J011.4489+58.0395 | 00:45:51.59 +58:02:18.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=VARIABLE SpType: M6II 2018MNRAS.475.2003D IRAS 00429+5745
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 20.0788* 00 45 52.94 +58 02 26.8 9.4 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
ATO J011.4489+58.0395,2461119.5788,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J011.4489+58.0395 20260320.0788 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:52.94 +58:02:26.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 9.52 00:48:53.39 +57:19:48.3
122.58645 -5.53996 galactic Cas Second-epoch detections are separated by 1.3" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 424651220519611008 | 00:48:52.64 +57:19:42.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 48 53.39 +57 19 48.3 9.5 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
Gaia DR3 424651220519611008,2461119.5788,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424651220519611008 20260320.0788 9.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:48:53.39 +57:19:48.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 10.46 00:44:58.70 +57:38:27.8
122.06407 -5.21981 galactic Cas Second-epoch detections are separated by 3.4" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 424719665120081408 | 00:44:57.87 +57:38:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 44 58.70 +57 38 27.8 10.5 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
Gaia DR3 424719665120081408,2461119.5788,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424719665120081408 20260320.0788 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:58.70 +57:38:27.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.04 00:44:56.01 +57:27:20.6
122.05333 -5.40493 galactic Cas Second-epoch detections are separated by 0.6" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 424710800307664640 | 00:44:55.47 +57:27:15.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 44 56.01 +57 27 20.6 11.0 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
Gaia DR3 424710800307664640,2461119.5788,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424710800307664640 20260320.0788 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:56.01 +57:27:20.6 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.11 00:46:21.51 +57:49:52.5
122.25325 -5.03381 galactic Cas Second-epoch detections are separated by 1.6" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 425051717633223552 | 00:46:20.54 +57:49:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 46 21.51 +57 49 52.5 11.1 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
Gaia DR3 425051717633223552,2461119.5788,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425051717633223552 20260320.0788 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:21.51 +57:49:52.5 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 50 29.28 +57 18 27.1 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
ASASSN-V J005028.46+571820.1,2461119.5788,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J005028.46+571820.1 20260320.0788 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:50:29.28 +57:18:27.1 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 50 06.91 +57 10 27.0 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
ASASSN-V J005006.33+571021.2,2461119.5788,11.54,0.05,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 J005006.33+571021.2 20260320.0788 11.54CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:50:06.91 +57:10:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.78 00:48:55.25 +57:01:37.6
122.58766 -5.84296 galactic Cas Second-epoch detections are separated by 0.5" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J012.2315+57.0360 | 00:48:54.67 +57:01:31.0 (Gaia DR3) | LPV (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 20.0788* 00 48 55.25 +57 01 37.6 11.8 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 J012.2315+57.0360,2461119.5788,11.78,0.05,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 J012.2315+57.0360 20260320.0788 11.78CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:48:55.25 +57:01:37.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.82 00:45:37.40 +57:38:02.0
122.15055 -5.22904 galactic Cas Second-epoch detections are separated by 1.2" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J011.3941+57.6235 | 00:45:36.73 +57:37:56.8 (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 20.0788* 00 45 37.40 +57 38 02.0 11.8 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 J011.3941+57.6235,2461119.5788,11.82,0.05,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 J011.3941+57.6235 20260320.0788 11.82CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:37.40 +57:38:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 46 29.05 +57 50 01.9 12.0 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
Gaia DR3 425051580190709376,2461119.5788,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425051580190709376 20260320.0788 12.02CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:29.05 +57:50:01.9 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 34 29.21 +64 32 50.6 11.9 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
V0660 Cas,2461119.5788,11.95,0.05,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
V0660 Cas 20260320.0788 11.95CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:29.21 +64:32:50.6 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.22 00:44:24.71 +58:01:00.6
121.99831 -4.84218 galactic Cas Second-epoch detections are separated by 1.5" and 1.2 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 | Gaia DR3 425104528549663616 | 00:44:23.80 +58:00:53.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M1 1981PASJ...33..107I [I81] M 491
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 20.0788* 00 44 24.71 +58 01 00.6 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
Gaia DR3 425104528549663616,2461119.5788,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425104528549663616 20260320.0788 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:24.71 +58:01:00.6 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 47 47.72 +57 43 14.4 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
Gaia DR3 425035568552706176,2461119.5788,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425035568552706176 20260320.0788 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:47:47.72 +57:43:14.4 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.59 00:45:48.57 +56:44:52.2
122.15601 -6.11544 galactic Cas Second-epoch detections are separated by 1.4" and 1.2 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 | Gaia DR3 424526803906787200 | 00:45:47.90 +56:44:44.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 45 48.57 +56 44 52.2 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
Gaia DR3 424526803906787200,2461119.5788,12.59,0.05,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
Gaia DR3 424526803906787200 20260320.0788 12.59CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:48.57 +56:44:52.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.71 00:45:39.74 +56:58:20.4
122.14081 -5.89054 galactic Cas Second-epoch detections are separated by 1.8" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 424624557361556864 | 00:45:38.67 +56:58:11.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 45 39.74 +56 58 20.4 12.7 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
Gaia DR3 424624557361556864,2461119.5788,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424624557361556864 20260320.0788 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:39.74 +56:58:20.4 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 51 36.62 +62 56 22.1 12.7 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,2461119.5788,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0788 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:51:36.62 +62:56:22.1 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 43 53.24 +61 53 18.3 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
Gaia DR3 511486250835935744,2461119.5788,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511486250835935744 20260320.0788 12.90CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:53.24 +61:53:18.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 50 31.14 +56 57 51.3 13.0 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 1714754,2461119.5788,13.02,0.05,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 1714754 20260320.0788 13.02CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:50:31.14 +56:57:51.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 32 56.84 +66 00 52.0 13.6 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
target,2461119.5788,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0788 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:56.84 +66:00:52.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 02 44 30.77 +65 04 14.5 14.0 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,2461119.5788,14.02,0.05,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 20260320.0788 14.02CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:44:30.77 +65:04:14.5 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 33 06.05 +65 23 55.5 13.9 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
target,2461119.5788,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0788 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:33:06.05 +65:23:55.5 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 02 44 44.99 +64 06 47.7 14.1 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
Gaia DR3 467669402499921920,2461119.5788,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 467669402499921920 20260320.0788 14.08CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:44:44.99 +64:06:47.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 14.16 01:41:55.72 +57:32:30.8
129.68963 -4.66588 galactic Cas Second-epoch detections are separated by 5.9" and 0.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:41:55.72 +57:32:30.8 (user input) | T | P | (position from user input) J-Ks=0.728+/-0.192 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 01 41 55.72 +57 32 30.8 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.5788,14.16,0.05,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 20260320.0788 14.16CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:55.72 +57:32:30.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 55 36.82 +58 30 09.4 14.1 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
target,2461119.5788,14.12,0.05,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
target 20260320.0788 14.12CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:36.82 +58:30:09.4 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 46 33.64 +58 55 29.0 14.3 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
target,2461119.5788,14.30,0.05,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 20260320.0788 14.30CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:33.64 +58:55:29.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 55 51.31 +64 01 15.7 14.3 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
target,2461119.5788,14.26,0.05,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 20260320.0788 14.26CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:51.31 +64:01:15.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 14 49.78 +57 23 46.2 13.0 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 J011449.70+572341.1,2461119.5788,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J011449.70+572341.1 20260320.0788 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:14:49.78 +57:23:46.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.88 00:59:00.26 +59:32:05.0
123.89248 -3.32291 galactic Cas Second-epoch detections are separated by 0.6" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426053574582188672 | 00:58:59.80 +59:32:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 59 00.26 +59 32 05.0 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
Gaia DR3 426053574582188672,2461119.5788,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426053574582188672 20260320.0788 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:59:00.26 +59:32:05.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 47 23.09 +66 08 02.9 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 J0047219+660805,2461119.5788,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0047219+660805 20260320.0788 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:47:23.09 +66:08:02.9 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 45 35.78 +63 07 06.0 12.8 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
ASASSN-V J014535.87+630702.7,2461119.5788,12.80,0.05,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
ASASSN-V J014535.87+630702.7 20260320.0788 12.80CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:35.78 +63:07:06.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 11.59 01:29:32.81 +63:18:25.8
127.19623 0.75138 galactic Cas Second-epoch detections are separated by 1.4" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512422794227736704 | 01:29:32.93 +63:18:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8Ib 1987ApJS...64..241S NGC 559 14
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 20.0788* 01 29 32.81 +63 18 25.8 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
Gaia DR3 512422794227736704,2461119.5788,11.59,0.05,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
Gaia DR3 512422794227736704 20260320.0788 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:29:32.81 +63:18:25.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 23 06.53 +66 51 38.1 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
target,2461119.5788,13.05,0.05,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 20260320.0788 13.05CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:23:06.53 +66:51:38.1 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.38 00:49:44.62 +56:57:26.4
122.69973 -5.91365 galactic Cas Second-epoch detections are separated by 2.6" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 423885479393057664 | 00:49:44.07 +56:57:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 49 44.62 +56 57 26.4 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
Gaia DR3 423885479393057664,2461119.5788,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 423885479393057664 20260320.0788 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:49:44.62 +56:57:26.4 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 25 02.46 +61 04 42.9 9.7 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
BT Cas,2461119.5788,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BT Cas 20260320.0788 9.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:25:02.46 +61:04:42.9 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 46 13.29 +57 26 24.2 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
ASASSN-V J004612.81+572618.1,2461119.5788,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J004612.81+572618.1 20260320.0788 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:13.29 +57:26:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.22 02:45:28.04 +64:13:14.1
134.94215 4.04090 galactic Cas Second-epoch detections are separated by 0.3" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 467764067877856896 | 02:45:28.27 +64:13:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.910+/-0.026 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 02 45 28.04 +64 13 14.1 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
Gaia DR3 467764067877856896,2461119.5788,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 467764067877856896 20260320.0788 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:45:28.04 +64:13:14.1 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 02 32 45.91 +56 29 31.8 13.0 U Per 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
LR Per,2461119.5788,13.02,0.05,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
LR Per 20260320.0788 13.02CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:32:45.91 +56:29:31.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 42 24.91 +59 07 07.8 11.9 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
ASASSN-V J004223.97+590701.7,2461119.5788,11.89,0.05,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 J004223.97+590701.7 20260320.0788 11.89CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:24.91 +59:07:07.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.32 00:53:52.68 +57:38:01.2
123.25984 -5.23653 galactic Cas Second-epoch detections are separated by 0.4" and 1.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J013.4677+57.6372 | 00:53:52.63 +57:37:57.5 (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 20.0788* 00 53 52.68 +57 38 01.2 12.3 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
ATO J013.4677+57.6372,2461119.5788,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J013.4677+57.6372 20260320.0788 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:53:52.68 +57:38:01.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 09 49.99 +65 08 27.6 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+650828,2461119.5788,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0109489+650828 20260320.0788 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:09:49.99 +65:08:27.6 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.18 00:59:46.89 +57:17:51.8
124.06401 -5.55569 galactic Cas Second-epoch detections are separated by 1.2" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 424119847168139904 | 00:59:46.86 +57:17:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 59 46.89 +57 17 51.8 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
Gaia DR3 424119847168139904,2461119.5788,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424119847168139904 20260320.0788 12.18CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:59:46.89 +57:17:51.8 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 46 18.28 +59 37 43.7 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
ASASSN-V J004617.85+593740.1,2461119.5788,11.56,0.05,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 J004617.85+593740.1 20260320.0788 11.56CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:18.28 +59:37:43.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 37 01.11 +63 08 02.2 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
TY Cas,2461119.5788,12.25,0.05,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
TY Cas 20260320.0788 12.25CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:01.11 +63:08:02.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 47 14.75 +57 40 32.2 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
ASASSN-V J004714.69+574033.2,2461119.5788,12.15,0.05,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
ASASSN-V J004714.69+574033.2 20260320.0788 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:47:14.75 +57:40:32.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 02 18 52.15 +62 48 16.9 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
NSVS 1867220,2461119.5788,12.91,0.05,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 1867220 20260320.0788 12.91CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:18:52.15 +62:48:16.9 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.55 00:43:47.49 +58:17:15.9
121.92401 -4.56903 galactic Cas Second-epoch detections are separated by 1.5" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 425126450062421248 | 00:43:47.01 +58:17:11.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 43 47.49 +58 17 15.9 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
Gaia DR3 425126450062421248,2461119.5788,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425126450062421248 20260320.0788 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:47.49 +58:17:15.9 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 43 45.71 +58 00 44.2 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
LAMOST J004346.89+580104.2,2461119.5788,12.23,0.05,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
LAMOST J004346.89+580104.2 20260320.0788 12.23CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:45.71 +58:00:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 12 11.36 +59 57 30.0 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+595728,2461119.5788,12.44,0.05,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 20260320.0788 12.44CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:12:11.36 +59:57:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0788 2461119.5788 12.46 00:43:08.62 +58:24:43.2
121.84267 -4.44221 galactic Cas Second-epoch detections are separated by 1.4" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 425131122986775296 | 00:43:07.95 +58:24:37.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0788* 00 43 08.62 +58 24 43.2 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
Gaia DR3 425131122986775296,2461119.5788,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425131122986775296 20260320.0788 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:08.62 +58:24:43.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 48 26.10 +57 03 00.7 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
target,2461119.5788,13.16,0.05,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 20260320.0788 13.16CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:48:26.10 +57:03:00.7 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 53 33.87 +57 49 00.1 11.7 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 J005333.38+574855.1,2461119.5788,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J005333.38+574855.1 20260320.0788 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:53:33.87 +57:49:00.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 02 01 09.58 +61 03 41.6 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 J0201098+610342,2461119.5788,13.08,0.05,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 J0201098+610342 20260320.0788 13.08CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:01:09.58 +61:03:41.6 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 05 28.21 +65 58 56.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0888 Cas,2461119.5788,11.24,0.05,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
V0888 Cas 20260320.0788 11.24CV 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:05:28.21 +65:58:56.5 ;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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 00 54 20.03 +57 41 48.8 13.0 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,2461119.5788,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0788 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:54:20.03 +57:41:48.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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 20.0788* 01 14 53.88 +63 36 45.3 12.1 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
V0724 Cas,2461119.5788,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0724 Cas 20260320.0788 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:14:53.88 +63:36:45.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_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_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.73552235 23.12.2025 05:38:59.131 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
First image: 2461032.73552235 23.12.2025 05:38:59.131 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
Last image: 2461119.57908815 20.03.2026 01:53:43.216 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 37
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 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): 28399
Objects passed selection criteria: 28291
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 21469.8
Average stars matched: 20869 (97.2019 %)
Memory usage VmPeak: 131940 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 21:20:23 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.73552235 23.12.2025 05:38:59.131 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
First image: 2461032.73552235 23.12.2025 05:38:59.131 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
Last image: 2461119.57908815 20.03.2026 01:53:43.216 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 793
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 51 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): 190259
Objects passed selection criteria: 189842
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 146805
Average stars matched: 141549 (96.4199 %)
Memory usage VmPeak: 2011436 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 21:25:17 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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: 2461119.57859100
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits'
wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits'
wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits'
wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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 01:42:51.042 +61:59:50.50
Second-epoch image center 01:42:21.015 +61:59:49.27
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 01:42:51.042 +61:59:50.50
Second-epoch image center 01:42:20.106 +61:59:52.32
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 01:42:21.015 +61:59:49.27
Second-epoch second image center 01:42:20.106 +61:59:52.32
Angular distance between the image centers 0.00197 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits &> /tmp/tmp.nSoC5jSYiL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits &> /tmp/tmp.0B5h4YZuW2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits &> /tmp/tmp.wmFjhIKf4y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits &> /tmp/tmp.OuyoGKHAar
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits and wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits and wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits and wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits) and catalog (wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat) found
'wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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 16291 out of 30008 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.954832
a=0.000000 b=1.000000 c=22.954832
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
2.2 pix Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
Limiting magnitude estimates:
15.2 mag. Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
15.2 mag. Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
14.1 mag. fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
14.2 mag. fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.nSoC5jSYiL (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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits' -> 'wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3505, passed=30008
Got 30008 stars (including 26471 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat
util/solve_plate_with_UCAC5 got 30008 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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: 0.38"
Estimated accuracy of the plate solution: 0.35"
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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits -region wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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.0B5h4YZuW2 (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_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits' -> 'wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3466, passed=30019
Got 30019 stars (including 26515 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat
util/solve_plate_with_UCAC5 got 30019 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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: 0.38"
Estimated accuracy of the plate solution: 0.34"
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_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits -region wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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.wmFjhIKf4y (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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.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_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1222, passed=12899
Got 12899 stars (including 11667 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat
util/solve_plate_with_UCAC5 got 12899 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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 967 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits -region wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.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.OuyoGKHAar (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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1272, passed=13502
Got 13502 stars (including 12222 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat
util/solve_plate_with_UCAC5 got 13502 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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.74"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.74"
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 969 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_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits -region wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits'
Saving fully-calibrated image wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52160.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52192.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52239.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 51903_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 51903_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 51904_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 51904_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:49:09.25 +63:28:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 3.057 467577666298548480 042.28923104418 +63.47231961690 10.9258 10.4219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51906_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 51906_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:39:03.00 +64:11:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 2.870 526970776168059520 009.76411573053 +64.19018071473 10.1031 9.7207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51909_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 51909_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 51911_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 51911_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 51982_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 51982_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:25:02.44 +61:04:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.54, MAG_FAINT_SEARCH_LIMIT=10.52)GAIADR2_OUTPUT=# 2.468 510684255881914752 021.25911182939 +61.07809768266 10.4950 8.7952 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52005_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 52005_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:19:06.79 +57:08:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.87, MAG_FAINT_SEARCH_LIMIT=10.85)GAIADR2_OUTPUT=# 5.537 458374822696458624 034.77902994100 +57.15123513662 10.3768 10.0529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52054_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52054_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 52072_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 52072_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:19:46.43 +58:12:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.49, MAG_FAINT_SEARCH_LIMIT=11.47)GAIADR2_OUTPUT=# 0.191 413827387540175360 019.94342845582 +58.20719933433 10.5311 10.2519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52087_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 52087_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:19:16.39 +57:10:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.64, MAG_FAINT_SEARCH_LIMIT=11.62)GAIADR2_OUTPUT=# 1.537 458375338092496768 034.81904201847 +57.18312008816 10.7388 10.3801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52160_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 52160_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:33:24.29 +60:39:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 0.662 509862924996841984 023.35139623571 +60.66242410040 11.2048 10.9125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52162_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52162_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 52177_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52177_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 52181_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 52181_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:05:28.17 +65:58:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 5.371 525946443646335104 016.36406548690 +65.98322508575 10.7226 8.9085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52192_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 52192_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:18:52.56 +57:06:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 3.396 458371730320067712 034.72023995337 +57.11261691123 11.3157 11.0364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52199_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 52199_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:19:09.48 +57:06:25.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)
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Considering the candidate 52239_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 52239_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 52280_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 52280_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 05942_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 05942_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 10718_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 10718_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 22543_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 22543_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 04699_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 04699_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 07175_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 07175_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 22s
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 ####
01:23:00.84 +64:39:24.5
00:46:55.79 +63:56:06.7
02:30:27.23 +62:31:46.5
01:28:36.98 +62:16:38.8
00:54:54.27 +58:33:50.7
00:35:58.92 +65:01:35.6
00:32:56.21 +65:13:04.3
00:46:12.54 +57:13:12.6
02:38:00.96 +63:01:46.6
00:46:54.08 +56:40:16.0
00:45:28.44 +57:19:14.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits exists and is non-empty
wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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 01:42:51.042 +61:59:50.50
Second-epoch image center 01:42:21.015 +61:59:49.27
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 01:42:51.042 +61:59:50.50
Second-epoch image center 01:42:20.106 +61:59:52.32
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 01:42:21.015 +61:59:49.27
Second-epoch second image center 01:42:20.106 +61:59:52.32
Angular distance between the image centers 0.00197 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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits &> /tmp/tmp.DwlAYy2iuf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits &> /tmp/tmp.VpWLiwPxiM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits &> /tmp/tmp.NRucNldbSL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits &> /tmp/tmp.Cukf33uXqb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits and wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits and wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits and wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits) and catalog (wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat) found
'wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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 16860 out of 206946 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.798772
a=0.000000 b=1.000000 c=22.798772
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 661 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
2.0 pix Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
2.3 pix fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
2.3 pix fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
Limiting magnitude estimates:
15.4 mag. Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
15.4 mag. Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
14.2 mag. fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
14.3 mag. fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.DwlAYy2iuf (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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits' -> 'wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=32108, passed=206911
Got 206911 stars (including 174495 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat
util/solve_plate_with_UCAC5 got 206911 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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: 0.39"
Estimated accuracy of the plate solution: 0.36"
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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits -region wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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.VpWLiwPxiM (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_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits' -> 'wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=32059, passed=205479
Got 205479 stars (including 173113 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat
util/solve_plate_with_UCAC5 got 205479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits -region wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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.NRucNldbSL (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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.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_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=7855, passed=87192
Got 87192 stars (including 79238 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat
util/solve_plate_with_UCAC5 got 87192 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 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: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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: 0.66"
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 969 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_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits -region wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.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.Cukf33uXqb (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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=8551, passed=91121
Got 91121 stars (including 82467 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat
util/solve_plate_with_UCAC5 got 91121 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 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: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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: 0.66"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 969 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_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits -region wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/wcs_Cas-03-Q2b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits
Saving fully-calibrated image wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/wcs_Cas-03-Q2b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-00_20.00sec_-15.00C_LIGHT_0004.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.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_2026-03-19_CI_Cas-03-Q2b1x1_211757_TTUQ2b1x1_7053_U7mAKDXn/wcs_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005.fits
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out204323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out218533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out218809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out231046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234367.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out237049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out237071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out237079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out234605.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out235138.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out05633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out206409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234579.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66720.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 143s
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: 57s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234243_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234243_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:02:25.02 +59:53:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.866 507928265566692864 030.60515075187 +59.89013522204 14.0999 13.3172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234249_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234249_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:45:21.04 +65:13:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234253_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234253_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:31:09.51 +60:23:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.127 509841106569061248 022.79126710445 +60.39616187425 13.7481 13.1876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234255_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234255_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:46:09.32 +58:29:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.534 506021265728127744 026.53948967685 +58.49785793896 13.8439 12.9962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234257_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234257_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:59:07.29 +61:45:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.137 508655077113067776 029.77980078725 +61.74961105124 13.8667 13.2254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234259_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234259_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:49:29.37 +63:29:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.916 467577906816708608 042.37275556219 +63.48291242568 13.7165 13.0462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234264_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234264_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:54:36.84 +59:08:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.056 506344625229184896 028.65385565695 +59.14195188830 13.8151 13.3506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234276_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234276_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234279_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234279_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:47:19.22 +63:30:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.185 467591891230034304 041.82988289797 +63.50326067020 13.5778 12.9330 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234280_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234280_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:47:16.43 +64:40:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.806 515838839411291648 041.81955909255 +64.67013228317 13.0355 11.9793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234284_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234284_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:19:17.19 +56:41:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.010 458324657477843456 034.82228118791 +56.69221241990 13.7473 13.1898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234286_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234286_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:40:53.98 +57:55:16.1 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 234287_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234287_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:55:48.50 +58:53:34.2 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 234289_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234289_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:26:12.52 +58:14:15.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 234292_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234292_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:28:40.83 +66:47:24.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
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Considering the candidate 234295_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234295_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:50:09.87 +57:10:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.174 505701720160986240 027.54263514376 +57.18111680706 13.6245 12.8143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234296_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234296_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:36:11.72 +59:50:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.039 509753283075176064 024.04876091343 +59.83711973609 13.5086 12.5707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234297_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234297_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:41:50.48 +61:48:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.229 511481440472455040 025.45933777705 +61.80429180063 13.0222 11.9019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234298_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234298_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:44:30.16 +64:14:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.302 515803002203660672 041.12690655944 +64.23585035767 12.9060 11.6220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234300_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234300_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234301_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234301_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:46:49.83 +61:07:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.950 427371648504300544 011.70858484044 +61.12824754324 12.6391 12.1098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234303_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234303_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 234304_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234304_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:47:54.40 +60:24:00.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
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Considering the candidate 234305_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234305_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:44:27.96 +60:41:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.095 509678546343520896 026.11699069431 +60.68979781333 14.2469 13.7162 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234310_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234310_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:47:18.78 +63:38:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 4.060 512068064285526784 026.83066913927 +63.63662862749 13.4108 12.6889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234311_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234311_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:21:00.17 +57:02:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.075 458359532612977280 035.25122573166 +57.03670611739 13.5991 13.2029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234321_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234321_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:17:00.37 +57:06:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.496 413417097905558016 019.25152270411 +57.11427920507 13.2984 12.7626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234329_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234329_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:48:03.13 +63:35:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.742 523877575082694400 012.01463618109 +63.59769365078 12.6047 12.0690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234330_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234330_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:14.62 +64:24:41.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 234332_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234332_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:07:15.49 +59:12:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.358 426161124862485376 016.81671025137 +59.20604502133 13.2581 12.6114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234333_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234333_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:32.62 +59:22:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.420 425466199154191232 010.38879473821 +59.37331406718 12.4334 11.9435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234334_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234334_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:45:51.70 +65:15:23.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 234337_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234337_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:48:24.98 +58:56:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 4.225 425224474095600256 012.10432463556 +58.94061077713 12.5333 11.9702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234338_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234338_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:32:23.81 +60:27:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.742 509836330565349504 023.10070954870 +60.45484867181 13.1128 12.3556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234339_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234339_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:46:15.95 +60:06:19.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 234340_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234340_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:36:20.25 +65:22:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.497 527180057033270656 009.08419553745 +65.36825366271 12.3651 11.6885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234342_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234342_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:14:56.08 +60:30:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.786 510401135941584384 018.73287903638 +60.51436411626 13.2499 12.7039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234343_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234343_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 234344_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234344_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234345_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234345_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:47:40.55 +58:54:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.896 425225646627357056 011.91800329204 +58.91355894960 12.5445 11.9892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234346_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234346_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234347_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234347_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:56:13.04 +56:55:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.484 424192548069645696 014.05577597979 +56.92813168181 12.7368 12.2379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234348_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234348_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:44:56.45 +57:49:44.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)
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Considering the candidate 234349_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234349_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:47:19.73 +58:19:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 5.035 425093773950340480 011.83025600868 +58.32590967090 12.2543 11.6080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234350_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234350_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:36:35.43 +62:15:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.545 430664380894719232 009.14821648840 +62.25869872619 12.4184 12.0655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234351_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234351_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:01:30.69 +65:05:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.115 518162107484452224 030.37739292442 +65.09376994290 12.8370 11.7418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234355_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234355_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:26.65 +64:01:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.291 523962924673970688 010.35902924526 +64.01757538124 12.3365 11.6775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234358_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234358_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:45:48.72 +64:12:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.875 524048063801168512 011.45398832309 +64.21578944659 12.3079 11.7856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234359_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234359_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:33:58.60 +63:47:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 5.752 430916817587200512 008.49148931957 +63.79701920230 12.1462 11.5013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234362_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234362_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:43:56.59 +63:49:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 3.722 523944542214073472 010.98344802387 +63.82556012549 12.3260 11.7489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234365_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234365_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 234367_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234367_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:26.37 +59:34:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.057 425502792276445440 010.35984636958 +59.56682679386 12.4095 11.7873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234370_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234370_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:54:53.95 +65:09:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.663 524347646360716800 013.72253974265 +65.16053200321 12.7038 11.7885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234373_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234373_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:35:07.17 +64:05:31.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 234374_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234374_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:46:42.46 +61:09:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 1.133 511216217653553664 026.67726181557 +61.16442721824 13.0336 12.4982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234376_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234376_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:03:21.65 +57:48:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.503 505400861990660864 030.84098328439 +57.81266284785 12.6742 11.6943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234380_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234380_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:35:08.93 +57:20:04.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)
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Considering the candidate 234383_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234383_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:38:38.51 +62:58:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 4.371 430807523564147200 009.66203614717 +62.97307580614 12.3350 11.7538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234384_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234384_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:59:22.00 +56:57:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.742 424020165264213504 014.83999446894 +56.96518802782 12.5854 11.5405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234385_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234385_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:42:57.19 +58:43:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.166 425164864250616960 010.73944922499 +58.72280692021 12.2683 11.7289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234387_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234387_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:51:09.24 +57:06:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.225 423882795027341184 012.78911711249 +57.10883594500 12.4271 11.9123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234389_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234389_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:54:06.11 +56:56:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 4.165 424201344161714048 013.52485810005 +56.93727936864 12.5245 11.9926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234392_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234392_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:10.99 +61:27:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 0.253 427253833265818624 010.29591748432 +61.45675882903 12.3977 12.0050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234393_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234393_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:56.18 +59:41:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.802 425499317640882176 010.48414232779 +59.69455600972 12.4128 11.9642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234396_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234396_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:46.97 +64:50:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 3.147 527104366831521152 010.19404815369 +64.83698423545 12.1157 11.4693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234398_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234398_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234401_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234401_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:53:40.31 +56:55:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 3.066 424201795141620480 013.41884594710 +56.91854949907 12.9766 12.2497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234403_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234403_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:55:43.78 +59:00:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.840 425977948796163584 013.93203938572 +59.01177838164 12.8436 11.9516 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 234404_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234404_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:47:26.97 +65:16:52.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)
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Considering the candidate 234405_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234405_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 234406_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234406_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:42:40.82 +59:27:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 4.643 425486673257170176 010.67222000984 +59.45769309257 12.2139 11.6885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234407_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234407_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:34:46.36 +58:12:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.396 508992146148098176 023.69374257255 +58.20450864053 12.9819 12.5064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234408_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234408_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:21.90 +64:20:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.439 527063955478124416 010.08914259585 +64.34272756163 12.2217 11.6429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234411_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234411_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:20:40.37 +56:58:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.662 458357471028756864 035.16868261287 +56.97689519370 12.8927 12.5667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234413_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234413_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 234415_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234415_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234416_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234416_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234427_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234427_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:01.40 +62:39:08.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)
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Considering the candidate 234429_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234429_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:35:26.73 +64:49:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 4.379 527139409462770688 008.85955343013 +64.82075674338 11.9228 11.3584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234430_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234430_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:25.84 +61:07:27.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 234431_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234431_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234432_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234432_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:23:05.71 +57:10:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.121 458413408680121856 035.77399264312 +57.17737512574 13.2206 12.8594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234433_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234433_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:39:36.92 +61:46:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 3.793 427273383956608384 009.90235625412 +61.77079475995 11.8933 11.3775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234436_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234436_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:30:31.54 +57:48:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.718 458086883782556544 037.63185620360 +57.81461191673 12.6812 12.0735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234438_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234438_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:47:05.56 +63:33:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.543 523887436327451520 011.77475304487 +63.56371324470 12.2177 11.6905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234439_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234439_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 234441_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234441_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234446_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234446_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 234447_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234447_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:37:20.88 +63:01:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.455 430805908656369152 009.33649784185 +63.01702718863 12.0811 11.6027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234448_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234448_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:39:46.42 +61:48:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.817 427648867175451392 009.94502158051 +61.81272140616 12.0153 11.5022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234454_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234454_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:43.21 +65:20:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 3.126 527499022783482880 010.17850353802 +65.34355364552 11.8236 11.2936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234455_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234455_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:32:23.01 +65:39:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.308 527389758814330496 008.09300529846 +65.65626297199 11.8294 11.2134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234456_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234456_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:22.52 +62:27:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 4.781 427694252088704768 010.09098655848 +62.46390471486 11.9738 11.4543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234457_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234457_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:38:56.14 +64:44:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.713 527090932172932608 009.73313287999 +64.74496357609 11.8905 11.2095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234460_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234460_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:59.24 +60:04:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 3.088 427018125458948096 010.49840928515 +60.07539870166 12.0583 11.5471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234462_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234462_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234463_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234463_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 234464_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234464_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234465_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234465_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:33:27.11 +64:46:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 4.969 527056984752538624 008.36618113468 +64.78188641335 11.7781 11.0748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234466_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234466_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:47:00.82 +62:08:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.094 427705079705745024 011.75261694128 +62.14433726021 12.0317 11.5616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234469_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234469_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:36:01.99 +66:10:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.573 527618251077040768 009.00895567568 +66.18251610933 12.0418 11.5226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234471_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234471_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:54:01.73 +57:31:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.510 424249035479495680 013.50899309825 +57.53106940762 11.8113 10.9892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234472_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234472_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234473_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234473_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 234474_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234474_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234475_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234475_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:44:17.76 +65:43:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 4.150 524622764783464704 011.07208896700 +65.72871182797 11.9869 11.5006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234476_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234476_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 234478_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234478_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234479_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234479_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:35:51.69 +64:28:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.150 527036403269490688 008.96421858801 +64.47807914461 11.6513 10.9727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234481_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234481_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:38:53.69 +56:58:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 0.893 409812349030613504 024.72359513149 +56.97853739907 12.6997 12.2219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234482_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234482_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:43:46.05 +65:04:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.505 524489178425588608 010.94234721426 +65.07683999631 11.7005 10.8813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234483_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234483_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 234487_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234487_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 234488_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234488_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:37:47.24 +63:49:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.745 526941742188581248 009.44828842290 +63.83048528716 11.8135 11.2510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234489_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234489_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:15:14.73 +59:31:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.185 507297180254126464 033.81178786087 +59.52141280981 12.6714 12.0139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234490_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234490_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:54:58.94 +58:47:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.809 425951182558564864 013.74469566981 +58.79029769600 12.1166 11.4993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234491_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234491_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:39:22.82 +66:18:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.052 527657592975774336 009.84242229033 +66.30475977910 11.8150 11.2464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234493_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234493_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234494_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234494_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:43:32.38 +59:37:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.445 425495920328768640 010.88526335656 +59.62369461198 12.0304 11.6828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234495_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234495_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:37:09.72 +62:14:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.023 430667095314074496 009.28992639022 +62.24706115186 11.7033 10.9623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234496_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234496_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 234497_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234497_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234498_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234498_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:04:01.04 +56:52:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 3.465 424045320893632768 016.00345072891 +56.86677828565 12.1262 11.2774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234499_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234499_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 234501_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234501_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:07.09 +61:15:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.224 427224455688475264 010.02844082280 +61.25198739958 11.9048 11.3711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234502_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234502_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 234504_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234504_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234506_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234506_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234508_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234508_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 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 234510_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234510_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:55:58.36 +58:52:47.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
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Considering the candidate 234511_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234511_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:38:00.47 +63:58:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 4.866 526949988525746560 009.50299004447 +63.96980143339 11.6817 11.0747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234513_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234513_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:39:47.56 +61:15:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.291 427225172939512192 009.94666173490 +61.25927453978 11.9547 10.9907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234514_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234514_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:55:58.94 +57:04:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.724 424195679108079232 013.99632365764 +57.08085121413 11.9650 11.4573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234515_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234515_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:36:18.59 +62:22:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 5.547 430671974396804352 009.07516118496 +62.38102515378 11.3644 10.9193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234517_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234517_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:51:43.56 +57:15:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.604 505722885761443840 027.93155937839 +57.25086305424 12.6533 12.1467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234519_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234519_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:38:33.36 +60:57:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.246 427132096713782912 009.64084685162 +60.96315246744 11.7860 11.2985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234521_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234521_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:45:00.85 +58:09:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 4.346 425108544335385856 011.25475168612 +58.15697526193 12.1711 11.7015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234522_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234522_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:45:11.96 +58:56:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 5.436 425253065699444096 011.30253861122 +58.94352101890 11.8845 11.3603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234523_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234523_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234524_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234524_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:11.88 +59:52:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 4.698 425514508947023104 010.30192366837 +59.86750053892 11.6440 11.1369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234526_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234526_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 234528_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234528_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:35:39.54 +63:26:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 3.437 430855146162221952 008.91273972877 +63.44090027370 11.6845 11.1467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234529_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234529_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234530_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234530_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:44:22.02 +58:46:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234531_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234531_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:49.14 +61:16:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.267 427245037172885248 010.20561253526 +61.27213720743 11.7121 11.0983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234532_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234532_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:43:59.24 +61:55:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.088 511486800591721088 025.99643284695 +61.92187486255 12.4658 11.7423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234533_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234533_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:42.92 +65:21:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.486 527496720681013376 010.42810298647 +65.36258246130 11.7362 11.2087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234534_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234534_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 234535_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234535_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234536_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234536_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:42:40.72 +65:58:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 3.312 527632166769562624 010.66769469321 +65.97060654615 11.4615 10.8997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234537_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234537_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:41:26.58 +65:00:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.959 513048622500390528 025.36063882979 +65.00262333794 12.4307 11.8894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234538_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234538_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:42:52.93 +60:18:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.552 427039011874299648 010.72187645588 +60.31392285093 11.5454 10.7671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234539_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234539_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234540_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234540_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:16:20.57 +62:42:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.127 523029847312700672 019.08698223791 +62.70774523967 12.5087 11.9233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234542_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234542_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:38:38.15 +66:07:17.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)
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Considering the candidate 234543_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234543_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234544_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234544_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234547_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234547_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:55:14.55 +59:32:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.268 506368711405374592 028.81088846526 +59.53410366189 12.4828 11.9913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234548_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234548_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234549_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234549_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:27.50 +60:46:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 4.045 427114435808416768 010.11677212639 +60.76687571328 11.5817 11.0101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234550_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234550_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:14.73 +65:32:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 4.401 527525479782720768 010.31422851083 +65.53909117112 11.6499 11.1152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234553_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234553_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234554_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234554_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234555_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234555_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234556_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234556_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234557_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234557_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234558_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234558_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:47.64 +65:05:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 3.998 527487409192095744 010.45077676839 +65.09892149499 11.4948 10.8454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234559_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234559_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:47:49.34 +66:30:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.764 526174042554875648 011.95658130995 +66.50959147536 11.3806 10.7461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234560_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234560_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234561_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234561_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234562_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234562_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234566_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234566_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:12.16 +61:00:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.361 427212326701060608 010.05201749953 +61.00918326676 11.3204 10.4937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234567_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234567_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:38:32.39 +63:00:37.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)
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Considering the candidate 234568_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234568_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 234570_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234570_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 234574_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234574_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:37:48.88 +61:53:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 5.270 430280853189319552 009.45093247915 +61.88661157287 11.4631 11.0600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234576_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234576_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 234577_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234577_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234578_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234578_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234579_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234579_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234580_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234580_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234581_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234581_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:39:12.14 +65:08:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 5.270 527126941179509120 009.80404248153 +65.14302620066 11.1339 10.5512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234582_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234582_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 234584_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234584_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:52:12.18 +58:33:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.072 506223949521102976 028.05118775854 +58.55511461354 11.9476 11.1086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234585_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234585_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:42:47.44 +59:07:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234586_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234586_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:31:09.33 +65:06:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 4.441 527346671702603520 007.78596271581 +65.10369655939 10.9430 10.3858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234587_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234587_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234589_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234589_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234591_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234591_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:38.53 +60:20:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 5.458 427051729283933824 010.41353145303 +60.34474864503 11.2564 10.7561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234592_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234592_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 234594_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234594_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:02.78 +60:11:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 2.167 427070249184030208 010.01082972861 +60.18994555034 11.3113 10.8314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234595_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234595_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:43:07.25 +58:44:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234596_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234596_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234597_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234597_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 234599_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234599_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 234602_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234602_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:37:20.75 +61:36:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 0.929 430269828019265280 009.33663388802 +61.60197795449 11.0476 10.6412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234603_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234603_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:37:02.03 +62:24:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 5.388 430672764660803072 009.25579752868 +62.40190131924 11.1413 10.6205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234604_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234604_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:38:44.09 +62:54:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 3.867 430800685976264960 009.68141545445 +62.90685949813 10.9792 10.4625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234605_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234605_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:38:33.00 +62:53:11.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)
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Considering the candidate 234606_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234606_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:35:37.01 +62:35:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.616 430710732174591488 008.90473293219 +62.59287023265 10.9420 10.2850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234607_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234607_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:38:15.72 +64:52:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 4.973 527119210238338048 009.56875286550 +64.87861818712 11.0313 10.4291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234608_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234608_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:39:22.05 +61:37:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 5.541 427270703897129472 009.84506799788 +61.62939825403 11.0737 10.5792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234609_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234609_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:35:16.74 +62:36:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 1.629 430710972700875264 008.81940072042 +62.60696594625 11.0896 10.5786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234610_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234610_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:26:22.28 +57:24:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 2.977 458429660837322112 036.59426336294 +57.40483848009 12.1511 11.2126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234611_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234611_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234612_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234612_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 234615_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234615_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:50:46.00 +57:21:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234619_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234619_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234620_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234620_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:34:57.80 +62:51:53.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)
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Considering the candidate 234622_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234622_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:40:39.14 +60:33:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 4.396 427105467916822528 010.16537656249 +60.56635916608 11.2402 10.8039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234623_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234623_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234626_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234626_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234627_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234627_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234628_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234628_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:33:22.09 +63:30:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 4.933 430883630386248192 008.33930032057 +63.50777046461 10.6885 10.2580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234629_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234629_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:36:11.27 +63:44:05.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)
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Considering the candidate 234633_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234633_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234634_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234634_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234636_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234636_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234637_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234637_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:39:30.90 +61:06:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 1.824 427216587308522368 009.87977578988 +61.10657789916 10.5952 9.8660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234638_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234638_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:44:34.34 +66:16:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 2.836 527668862970279936 011.14115710492 +66.27871946216 10.6716 10.0348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234639_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234639_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234640_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234640_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234645_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234645_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234646_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234646_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:38:08.70 +64:39:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 3.737 527089660862659712 009.53513942768 +64.65381167505 10.2805 9.6667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234647_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234647_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:35:58.76 +65:01:34.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 234648_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234648_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234649_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234649_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 234650_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234650_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 234651_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234651_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:31:39.13 +64:40:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 0.819 527052414907360256 007.91353402817 +64.67916399309 9.7859 9.2511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234652_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234652_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:35:19.30 +62:32:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 5.790 430687230120567936 008.82701411066 +62.54389545117 9.8744 9.3412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234654_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234654_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:39:03.61 +64:11:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 2.848 526970776168059520 009.76411573053 +64.19018071473 10.1031 9.7207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234655_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234655_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:32:55.84 +65:13:03.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 234658_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234658_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:42:05.81 +64:22:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.26, MAG_FAINT_SEARCH_LIMIT=11.24)GAIADR2_OUTPUT=# 3.439 524067343919352960 010.52257984036 +64.37839560984 9.5888 9.0828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234659_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234659_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:19:33.57 +58:15:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.33, MAG_FAINT_SEARCH_LIMIT=11.31)GAIADR2_OUTPUT=# 3.126 413874563464017152 019.89045223765 +58.26739681352 10.7919 10.5508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234660_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234660_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:41:26.24 +64:19:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.10, MAG_FAINT_SEARCH_LIMIT=11.08)GAIADR2_OUTPUT=# 3.920 524061846361234048 010.35738258325 +64.32946449545 9.3259 8.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234663_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234663_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 234719_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234719_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234731_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234731_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234754_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234754_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:19:06.83 +57:09:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.04, MAG_FAINT_SEARCH_LIMIT=11.02)GAIADR2_OUTPUT=# 4.488 458374822696458624 034.77902994100 +57.15123513662 10.3768 10.0529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234809_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234809_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234811_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234811_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:46:12.67 +57:13:13.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 234904_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234904_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234917_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234917_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234919_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234919_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234925_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 234925_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 234979_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234979_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:48:56.63 +56:49:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 5.779 423862557141460608 012.23433321824 +56.81577483021 10.7686 9.7966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234985_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234985_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234989_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234989_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:45:28.56 +57:19:14.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 234994_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 234994_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235018_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235018_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235024_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235024_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235040_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235040_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235074_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235074_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235105_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235105_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235132_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235132_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235138_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235138_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:31:22.74 +56:53:00.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)
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Considering the candidate 235145_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235145_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235196_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235196_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:38:00.39 +57:56:46.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235212_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235212_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235213_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235213_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235215_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235215_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:16:47.28 +57:00:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.015 458534939073962240 034.19722833989 +57.00608030280 12.1554 11.7637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235223_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235223_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235282_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235282_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235292_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235292_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235295_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235295_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235297_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235297_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235302_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235302_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:56:38.64 +59:13:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.452 425941531775245952 014.15995759183 +59.21943779628 11.7692 10.9134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235323_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235323_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235331_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235331_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:31:32.22 +58:00:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 3.343 458094962625547136 037.88523363275 +58.00062044959 11.1664 9.9212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235337_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235337_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235353_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235353_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:56:22.53 +60:44:40.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 235364_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235364_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:17:59.13 +57:47:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.881 413463895869935872 019.49656676179 +57.79373770284 12.1325 11.4375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235366_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235366_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235376_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235376_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235384_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235384_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 235391_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235391_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235411_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235411_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:03:46.75 +61:03:19.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235419_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235419_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235422_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235422_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:10:13.63 +59:59:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.174 507518761901777792 032.55721581237 +59.99005800007 11.9834 11.0353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235430_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235430_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 235434_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235434_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235436_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235436_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235437_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235437_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235440_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235440_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:33:35.43 +60:40:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.233 509863676609683968 023.39823070864 +60.67741188327 11.8932 10.7716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235454_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235454_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235458_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235458_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 235462_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235462_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235467_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235467_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:43:30.05 +59:36:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.685 509512421306957952 025.87548772340 +59.60259470788 12.3632 11.7801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235505_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235505_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:58:16.22 +59:38:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.262 507862844627662720 029.56967079484 +59.65034352526 12.8236 12.4000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235521_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235521_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235523_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235523_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235532_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235532_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235545_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235545_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:19:12.21 +65:36:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.348 525310578028184960 019.80018901367 +65.60077235821 11.3353 9.8218 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235547_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235547_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235554_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235554_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235555_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235555_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:53:16.24 +61:08:54.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235559_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235559_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235592_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235592_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:46:48.37 +59:52:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.121 426827360193310720 011.70047974416 +59.87249897700 12.1089 11.0427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235614_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235614_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235615_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235615_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235621_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235621_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235636_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235636_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235661_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235661_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:17:57.56 +61:42:00.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 235678_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235678_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235685_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235685_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235698_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235698_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:04:32.57 +57:59:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 3.100 425631224681610752 016.13597827400 +57.98787296851 12.3462 11.3699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235703_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235703_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235706_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235706_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:02:26.10 +59:41:15.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)
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Considering the candidate 235719_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235719_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:51:36.97 +63:46:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 4.443 523811943680819456 012.90657506998 +63.77325828609 12.2820 11.7391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235721_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235721_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235724_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235724_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 235725_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235725_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235728_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235728_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235731_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235731_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235745_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235745_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235748_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235748_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235758_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235758_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235763_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235763_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235765_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235765_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235785_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235785_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:45:03.61 +57:26:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 5.349 424710731588189824 011.26311964143 +57.44543306989 11.9728 10.8748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235792_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235792_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235798_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235798_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:42:06.12 +60:34:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.768 465561402488979328 040.52617769464 +60.56672220508 12.7554 12.1568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235809_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235809_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:45:53.51 +61:11:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 235812_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235812_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:03:36.69 +61:03:03.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235814_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235814_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235815_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 235815_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 235818_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235818_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235830_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235830_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235847_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235847_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:37:00.15 +59:37:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 2.118 509562410424777344 024.25127619021 +59.63220667306 12.4133 11.4082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235851_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235851_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235857_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235857_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 235867_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235867_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235869_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235869_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235878_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235878_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:18:18.99 +57:42:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 2.855 413462555840435840 019.58032681643 +57.70683999945 12.5214 11.4847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235879_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235879_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235881_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235881_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235888_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235888_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235896_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235896_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:53:03.12 +60:35:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 4.277 427283966753665664 013.26168762177 +60.59655744026 12.7276 10.7966 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235909_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235909_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235920_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235920_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:05:03.62 +64:21:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 2.597 515060075945586176 031.26502482935 +64.36397361378 12.6511 11.9459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235929_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235929_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235943_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235943_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:22:23.19 +57:03:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.485 458406468013138432 035.59683416740 +57.05665903749 13.1120 12.6047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235944_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235944_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:04:16.28 +61:36:12.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235947_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235947_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235961_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235961_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:46:33.60 +61:16:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.927 511219378749345152 026.64035262574 +61.27991602603 12.8700 12.3321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235971_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235971_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:14:54.25 +61:34:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.005 510583895388980224 018.72680057787 +61.57802044564 12.6806 12.0675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235972_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235972_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:24:06.76 +59:43:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 2.934 510092379331612416 021.02959881370 +59.72909424910 13.0398 12.6733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235977_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235977_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235980_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235980_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:31:59.23 +56:40:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.433 457959894492316800 037.99678680792 +56.67649081603 12.9736 12.3483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235981_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235981_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:44:17.63 +61:53:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.249 511299058984645248 026.07399720013 +61.88759705431 12.7552 12.2125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235987_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235987_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:51:02.61 +64:49:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.567 518229590006827648 027.75942395447 +64.83128019779 12.9799 12.3873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235988_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235988_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:38:32.97 +60:48:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.067 509905634154578560 024.63764517723 +60.80015133430 13.1380 12.7581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235989_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235989_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 235995_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235995_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:44:32.25 +58:45:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.978 506449869104978432 026.13543101232 +58.76014886449 13.1796 12.7854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235998_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 235998_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236003_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 236003_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 236004_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236004_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236014_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236014_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:20:10.97 +58:12:09.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236016_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236016_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:00:51.80 +58:31:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.213 505508446637646592 030.21645161399 +58.52382030882 12.9664 12.6563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236017_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236017_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:10:54.56 +57:40:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.850 413555567649210240 017.72817167009 +57.67910970634 12.9060 12.3387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236020_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236020_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:07:13.34 +58:48:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 0.402 506981792216049408 031.80579880154 +58.81406044009 12.8551 12.3078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236022_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236022_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:16:08.14 +58:49:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.840 414094981181756928 019.03612126008 +58.82748339054 12.5405 11.5452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236024_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236024_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:50:31.71 +64:14:26.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236026_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236026_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:54:24.94 +57:43:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.756 506105309648141056 028.60408916862 +57.72685440303 13.2390 12.9759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236044_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236044_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236055_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236055_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:31:03.67 +66:05:04.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236061_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236061_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:13:30.19 +58:34:25.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236078_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236078_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:02:54.92 +64:24:59.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236079_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236079_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:23:23.59 +63:36:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.328 514342575887502464 035.84909384475 +63.60387735364 12.5425 11.4782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236095_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236095_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:20:18.20 +58:13:43.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236098_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236098_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:21:01.45 +57:11:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.954 458457389147259392 035.25594644844 +57.18673486538 13.1338 12.6601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236111_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236111_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236114_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236114_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236117_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236117_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:39:35.09 +57:10:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.402 409809806409817984 024.89732325541 +57.17213421973 12.6709 11.6110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236122_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236122_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:46:51.86 +56:49:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.792 424610293770527232 011.71435590025 +56.82694808040 12.5675 11.7988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236126_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236126_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:15:03.25 +60:08:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.498 510385708419381504 018.76137398125 +60.13512080209 13.3430 12.7037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236129_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236129_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:03:22.26 +60:32:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.038 426389823283672320 015.84479183776 +60.53697283435 13.0644 12.8077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236130_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236130_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:11:23.15 +61:21:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.175 507738973467195904 032.84658712924 +61.35187400451 12.6159 11.5379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236132_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236132_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236137_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236137_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236148_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236148_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236160_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236160_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236164_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236164_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236168_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236168_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236170_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 236170_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 236176_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236176_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236202_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236202_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:25:22.15 +63:20:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.216 514288390578556160 036.34245991615 +63.33780586068 12.5944 11.4581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236215_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236215_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236216_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236216_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:58:54.59 +57:16:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.898 505281019525448192 029.72783586218 +57.28252330323 13.1385 12.4945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236220_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236220_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:00:36.69 +58:30:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.611 505502498096525184 030.15329247123 +58.50591471848 12.8217 11.9729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236228_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236228_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236231_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236231_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:36:09.90 +59:08:53.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 236232_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236232_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:15:58.90 +63:12:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.665 514705689602995968 033.99603100661 +63.20679630645 12.9611 12.3771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236235_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236235_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236236_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236236_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236250_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236250_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236252_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236252_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236261_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236261_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236262_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236262_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:45:24.89 +61:16:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 5.610 465610880512792576 041.35396080967 +61.26975207589 13.1082 12.2115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236263_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236263_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236269_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236269_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236272_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236272_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:17:00.00 +57:02:24.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236279_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236279_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236285_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236285_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236286_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236286_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:25:09.96 +57:16:08.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 236289_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236289_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:27:49.82 +62:54:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.943 514075532000750720 036.95804085135 +62.91256327280 13.0065 12.4146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236292_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236292_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:29:33.84 +63:19:32.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)
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Considering the candidate 236297_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236297_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:45:09.34 +58:26:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.718 506066448786033792 026.28874475171 +58.43752663189 13.1797 12.2806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236307_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236307_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:36:15.34 +63:07:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.516 514130541941665024 039.06382923588 +63.12635865314 12.6838 11.7870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236308_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236308_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236319_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236319_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:04:26.47 +65:05:54.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236322_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236322_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:33:23.07 +57:44:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.329 412897028903336320 023.34630002000 +57.73961499900 12.9810 12.1035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236324_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236324_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236334_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236334_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236344_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236344_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236347_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236347_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:17:21.69 +59:22:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.274 507234508089993472 034.34003720349 +59.37580184164 13.3423 12.7680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236350_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236350_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236354_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236354_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:11:43.38 +66:29:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.732 518680321051630848 032.93223694266 +66.49610567916 13.1953 12.6051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236361_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236361_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236370_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236370_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236372_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236372_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:36:44.90 +57:01:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.411 412795014838312704 024.18741705538 +57.02845489341 12.8954 11.9620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236380_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236380_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:00:36.83 +63:32:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.271 523357845376882304 015.15346734270 +63.54609147647 12.3183 11.0743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236382_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236382_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:58:40.15 +59:16:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 4.368 507801031456497792 029.66851337035 +59.26623741797 13.3412 12.6434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236402_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236402_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:39:56.73 +60:52:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.807 509927482640610816 024.98639197744 +60.87027578284 12.2653 10.9831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236404_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236404_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 236406_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236406_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:19:03.66 +63:57:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.010 515127524109378816 034.76635535417 +63.96216816662 13.1052 12.4875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236410_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236410_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236422_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236422_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236425_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236425_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:30:09.01 +57:48:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.865 458089671225770752 037.53795425226 +57.81381937189 13.2540 12.7589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236430_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236430_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:35:50.31 +61:27:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.315 510005277399274368 023.96121378866 +61.45964520446 13.2733 12.6840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236434_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236434_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236445_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236445_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:16:36.24 +64:57:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.260 515428373678907264 034.15083013977 +64.96303378434 13.1119 12.4054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236461_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236461_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:01:14.97 +59:23:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.239 507816562059228544 030.31354850954 +59.38368853525 13.3052 12.6838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236462_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236462_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:24:01.44 +57:14:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.143 458412377887901312 036.00707646700 +57.24634946592 13.5568 12.9769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236465_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236465_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236468_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236468_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:22:13.37 +59:08:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.075 459200143609929216 035.55628920754 +59.13954670009 13.7928 13.2385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236478_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236478_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236486_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236486_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:01:36.87 +59:57:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.449 507939947877705600 030.40447218811 +59.95610706443 13.3816 12.7797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236488_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236488_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:19:57.78 +59:32:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.647 459224057987492224 034.99153878575 +59.54094426487 13.2778 12.7155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236501_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236501_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:54:18.61 +63:38:05.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 236503_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236503_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:11:52.36 +63:22:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.674 523210205882617856 017.96920422929 +63.37846665142 13.1563 12.6440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236506_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236506_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:38:08.21 +61:03:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.088 509945800689898496 024.53645990448 +61.06601549831 13.5746 13.1952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236513_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236513_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236515_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236515_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:35:54.20 +60:13:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 0.875 509780392908244224 023.97563084557 +60.22213797866 13.4292 12.9491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236523_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236523_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236529_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236529_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:06:09.61 +57:07:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.743 505132379297826944 031.54084257548 +57.12400908073 13.5463 12.8673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236535_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236535_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236537_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236537_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:17:00.89 +61:40:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.565 510587778039508352 019.25338061940 +61.67886736924 13.1966 12.5117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236538_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236538_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:52:48.64 +60:28:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.197 508121436018444800 028.20260553676 +60.47673221383 13.3356 12.4931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236542_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236542_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:38:16.28 +58:11:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 0.385 458148323296848512 039.56765774496 +58.19741870308 13.3853 12.8051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236545_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236545_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236548_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236548_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:07:40.55 +63:30:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.993 523312387443063168 016.92140212438 +63.50420394770 12.9413 11.8886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236551_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236551_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:33:12.20 +61:31:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.726 465535082930940160 038.29975528968 +61.51604620474 13.4370 12.8434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236558_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236558_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:40:43.57 +64:10:55.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)
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Considering the candidate 236566_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236566_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:58:04.22 +57:58:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 0.924 505383377188819840 029.51800723553 +57.98109816728 13.0545 12.1505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236569_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236569_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:12:48.67 +59:35:18.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
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Considering the candidate 236577_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236577_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:42:33.01 +63:52:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.071 512133141631534720 025.63708015871 +63.88281061709 13.2422 12.6004 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 236584_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236584_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:00:35.39 +58:32:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 0.310 505514390872372096 030.14742156599 +58.54263956534 13.8466 13.2844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236590_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236590_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236593_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236593_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236594_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236594_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:29:46.55 +58:31:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.060 458965226076600064 037.44244311091 +58.52678288863 13.4641 12.4966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236600_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236600_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:37:25.83 +60:41:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.023 509910062253273856 024.35957437478 +60.68983496187 13.1838 12.2602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236603_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236603_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 236604_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236604_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:39:23.96 +58:23:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.811 509053650078890880 024.85075682277 +58.38489070501 13.3169 12.4750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236614_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236614_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:27:52.45 +62:46:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.111 512378985553753856 021.96899826723 +62.77694931626 13.4421 13.0089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236621_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236621_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:24:28.05 +63:31:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.961 514361714262923136 036.11813246114 +63.52692569609 13.3222 12.2813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236624_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236624_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:20:14.50 +59:20:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.791 459212959792100480 035.06108979178 +59.33650085724 13.3437 12.7016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236627_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236627_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:58:04.87 +59:36:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.980 507862294871859328 029.51932920383 +59.61024734346 13.7065 13.0395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236630_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236630_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:37:44.69 +64:45:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.326 513064183156209536 024.43624931833 +64.76456259326 13.3761 12.7197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236635_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236635_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:46:50.65 +60:39:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.184 511164678045195008 026.71100154417 +60.65281066062 13.6732 13.1253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236637_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236637_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:43:06.81 +58:57:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.720 506467766229366272 025.77956337866 +58.95772488081 13.0963 12.1938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236644_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236644_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:33:47.71 +62:08:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.741 512289822038093312 023.44757177982 +62.14599209272 12.9306 11.7975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236648_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236648_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:41:51.03 +61:02:08.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236660_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236660_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236661_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236661_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:02:50.36 +60:14:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.807 507950874274333440 030.70908644465 +60.23330073972 13.5767 12.9091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236662_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236662_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:02:53.93 +60:15:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.282 507974445056106752 030.72507127407 +60.26141503043 13.0533 12.0731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236667_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236667_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236668_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236668_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:16:12.53 +62:42:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.929 523029851616185216 019.05297175742 +62.70737214812 13.2164 12.5858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236670_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236670_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236672_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236672_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:10:31.23 +60:57:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.851 507622326456919040 032.63010829315 +60.95120822338 13.6110 13.0028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236673_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236673_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236674_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236674_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:03:25.17 +57:50:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.134 505401347330523136 030.85563706404 +57.83678997919 13.5374 12.5654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236675_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236675_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236677_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236677_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236690_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236690_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:37:41.38 +58:37:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.303 509071654581514112 024.42352397305 +58.62561945068 13.6739 13.1233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236691_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236691_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236695_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236695_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:38:11.87 +61:01:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.534 509921542712795264 024.55065424724 +61.02376669093 13.1918 12.2662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236697_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236697_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236699_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236699_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236710_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236710_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:29:30.41 +60:40:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.097 465392730532552064 037.37615949945 +60.67792767616 13.5153 12.8403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236713_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236713_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:13:33.67 +57:53:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.189 413667133719433216 018.39141616752 +57.89508213946 13.0988 12.2426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236718_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236718_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236719_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236719_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236722_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236722_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236728_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236728_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236729_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236729_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236730_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236730_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:48:38.11 +61:49:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.155 511332143104791040 027.15857782551 +61.81904598779 12.7859 11.6380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236732_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236732_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236734_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236734_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236735_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236735_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:33:33.80 +60:18:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.722 465132833470541568 038.39043249075 +60.30369491780 13.9174 13.1039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236743_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236743_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236744_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236744_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:37:13.45 +58:38:30.9 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 236749_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236749_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236750_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236750_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:48:39.73 +59:09:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 3.025 506441966364217216 027.16714841081 +59.15502903525 13.0371 11.8781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236753_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236753_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:25:50.61 +61:32:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.843 513573742375820928 036.46142013017 +61.54600342105 13.3225 12.4677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236761_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236761_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236762_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236762_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:16:36.82 +64:56:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.293 515428274899736064 034.15194671424 +64.94466312831 13.5993 12.8997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236767_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236767_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:39:10.60 +63:44:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.150 515670201817309824 039.79429939831 +63.73287798878 13.4573 12.7540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236778_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236778_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:11:36.33 +57:37:15.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236779_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236779_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236784_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236784_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236786_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236786_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236787_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236787_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236793_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236793_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:14:52.88 +57:13:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.180 458554558484425856 033.72069740872 +57.23073292307 13.5761 12.9818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236794_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236794_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:14:00.26 +61:42:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.897 507763063945994112 033.50152998306 +61.70088156149 13.5621 12.8870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236795_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236795_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:54:34.76 +59:52:41.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 236798_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236798_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:14:29.86 +63:16:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.587 514709125576782976 033.62459601494 +63.27651112353 13.5133 12.8362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236804_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236804_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:44:56.62 +59:46:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.597 509611755310763136 026.23673320990 +59.77333289681 13.2838 12.3282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236820_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236820_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:59:10.51 +59:53:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.322 507895314581253888 029.79433991584 +59.89595088569 13.7952 13.3501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236821_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236821_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:00:23.93 +58:24:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 1.947 505500337739490816 030.10039891027 +58.40509626166 13.4583 12.6017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236830_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236830_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:48:29.59 +60:27:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.588 508156448593196416 027.12380764005 +60.46119371145 13.9375 13.5691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236832_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236832_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:44:06.54 +59:32:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.819 509508950973463552 026.02769855692 +59.53670405092 13.2104 12.2670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236834_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236834_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:43:12.68 +64:00:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 3.062 512140082298787584 025.80374330274 +64.01341524964 13.5560 12.8742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236842_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236842_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:54:30.32 +59:06:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.731 506344109833135616 028.62725042392 +59.10959655575 14.1495 13.6159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236847_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236847_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236848_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236848_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 236853_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236853_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236860_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 236860_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 236862_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236862_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236863_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236863_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236866_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236866_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:36:16.19 +57:44:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.583 458111386578384896 039.06837506124 +57.74639171097 13.4112 12.6867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236869_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236869_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:31:32.29 +61:02:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.779 510639897457891072 022.88531628927 +61.03898371859 13.6194 13.2113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236881_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236881_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236886_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236886_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236887_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236887_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236888_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236888_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:38:05.86 +61:04:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 0.958 509945869409369216 024.52451149061 +61.07062331621 13.5927 12.6651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236889_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236889_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:39:36.33 +60:53:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.746 509928483381902208 024.90168924326 +60.89739004049 13.8216 13.4301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236898_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236898_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236906_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236906_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236914_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236914_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236926_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236926_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:16:58.11 +58:17:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.660 458750924389421824 034.24220511870 +58.28490202677 13.7865 13.0663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236932_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236932_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236936_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236936_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236939_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236939_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:27:56.16 +62:46:07.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)
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Considering the candidate 236947_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 236947_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 236948_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236948_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236951_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236951_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236952_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236952_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236958_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236958_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236964_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236964_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236968_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236968_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:59:05.94 +59:55:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.848 507895623818884608 029.77468263229 +59.92662375336 13.3263 12.3938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236977_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236977_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236980_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236980_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:23:55.02 +66:08:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.627 525398367159969024 020.97753813118 +66.14526966832 13.6568 11.4304 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236982_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 236982_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 236985_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236985_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236986_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236986_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236989_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236989_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 236994_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 236994_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237004_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237004_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237005_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237005_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237007_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237007_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 237012_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 237012_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 237017_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237017_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237018_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237018_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237029_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237029_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237035_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237035_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237036_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237036_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237037_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237037_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237039_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237039_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237043_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237043_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237046_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237046_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237049_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237049_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:49:06.29 +65:23:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.420 518325865996846336 027.27689445834 +65.39533923730 13.7094 12.9107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 237052_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237052_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237058_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237058_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 237065_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237065_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237066_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237066_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237071_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237071_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:56:25.37 +62:05:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.066 508724483786831872 029.10570203568 +62.09170385753 13.4002 12.3491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 237072_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237072_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237079_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237079_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:12:34.64 +58:23:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 1.615 506813395137492864 033.14470312571 +58.38326220065 14.1214 13.6226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 237087_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237087_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237094_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237094_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237095_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237095_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237099_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237099_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237106_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 237106_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 237109_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237109_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 237110_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 237110_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 237115_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237115_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237118_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237118_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237119_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237119_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237120_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237120_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237122_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237122_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237123_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237123_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237126_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237126_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237128_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237128_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237130_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237130_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237138_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237138_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237139_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237139_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237144_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237144_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237145_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237145_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237146_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237146_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237148_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237148_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237149_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237149_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237150_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237150_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237156_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237156_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237157_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237157_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237158_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 237158_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 237166_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 237166_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 237169_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237169_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237173_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237173_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237175_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237175_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237176_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237176_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237179_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237179_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 237186_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 237186_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 162527_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 162527_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 143117_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 143117_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 218533_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 218533_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:07:46.29 +57:44:58.7 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 219261_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 219261_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:49:28.63 +57:29:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.725 424278760957375616 012.36881296543 +57.49404030133 11.5606 10.7761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 10462_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 10462_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
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Considering the candidate 20125_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 20125_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 48353_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 48353_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:46:55.64 +63:56:06.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 66720_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 66720_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65766_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 65766_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05633_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 05633_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206409_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 206409_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 231665_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 231665_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 110486_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 110486_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 231046_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 231046_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:02:02.22 +62:41:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.616 508824504983934208 030.50894759146 +62.69179528851 13.4614 12.8394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168792_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 168792_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13560_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 13560_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17040_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 17040_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174012_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 174012_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148899_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 148899_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170564_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 170564_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28705_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 28705_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85948_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 85948_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:28:37.10 +62:16:38.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161600_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 161600_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137512_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 137512_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60977_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 60977_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197357_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 197357_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 173416_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 173416_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38778_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 38778_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:23:00.88 +64:39:24.2 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58714_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 58714_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189379_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 189379_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183115_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 183115_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120737_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 120737_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227813_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 227813_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:38:00.94 +63:01:46.2 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135162_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 135162_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58234_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 58234_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 02:30:27.23 +62:31:46.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219046_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 219046_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:56:39.25 +57:22:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 4.819 424230103263662080 014.16230400185 +57.37445066229 12.2261 11.4642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218809_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 218809_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 01:28:56.58 +66:20:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.011 525417539891790976 022.23690079610 +66.33811972972 11.9675 10.9431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191644_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 191644_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:54:54.38 +58:33:52.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204323_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 204323_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
**** FOUND 00:51:41.07 +56:54:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 4.281 423876129238111488 012.91938898711 +56.91455956232 12.0186 11.1250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192120_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 192120_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159744_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 159744_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174646_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 174646_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100625_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 100625_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187629_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 187629_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14781_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 14781_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171566_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 171566_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59014_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
Preparing report for the candidate 59014_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153479_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005
The candidate 153479_fd_Cas-03-Q2b1x1_2026-03-19_20-53-43_20.00sec_-15.00C_LIGHT_0005 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
make_report_in_HTML.sh Phase 2 (HTML assembly): 25s
make_report_in_HTML.sh TOTAL: 225s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:23:00.84 +64:39:24.5
00:46:55.79 +63:56:06.7
02:30:27.23 +62:31:46.5
01:28:36.98 +62:16:38.8
00:54:54.27 +58:33:50.7
00:35:58.92 +65:01:35.6
00:32:56.21 +65:13:04.3
00:46:12.54 +57:13:12.6
02:38:00.96 +63:01:46.6
00:46:54.08 +56:40:16.0
00:45:28.44 +57:19:14.0
01:23:06.53 +66:51:38.1
02:01:09.58 +61:03:41.6
00:47:23.09 +66:08:02.9
01:25:02.46 +61:04:42.9
01:12:11.36 +59:57:30.0
00:46:18.28 +59:37:43.7
00:59:00.26 +59:32:05.0
01:05:28.21 +65:58:56.5
00:42:24.91 +59:07:07.8
00:48:26.10 +57:03:00.7
00:59:46.89 +57:17:51.8
01:14:49.78 +57:23:46.2
00:46:13.29 +57:26:24.2
02:45:28.04 +64:13:14.1
00:53:52.68 +57:38:01.2
00:54:20.03 +57:41:48.8
00:47:14.75 +57:40:32.2
02:32:45.91 +56:29:31.8
00:53:33.87 +57:49:00.1
00:43:45.71 +58:00:44.2
00:43:47.49 +58:17:15.9
00:43:08.62 +58:24:43.2
00:49:44.62 +56:57:26.4
00:39:24.46 +64:30:15.8
00:37:33.55 +62:02:14.3
00:39:37.31 +66:00:20.5
00:49:24.50 +58:00:18.0
00:38:07.46 +61:40:25.8
00:42:46.79 +65:05:55.8
00:35:09.74 +66:10:21.1
00:36:44.04 +62:48:52.5
00:37:26.01 +64:50:45.9
00:40:27.59 +64:33:43.2
00:37:18.58 +64:11:56.4
00:33:03.73 +64:29:55.5
00:35:10.32 +65:28:35.7
00:37:14.10 +64:34:40.8
00:36:14.79 +64:20:13.2
00:36:56.00 +63:24:13.7
00:30:22.65 +65:18:31.4
00:37:07.51 +62:10:06.0
00:37:12.58 +65:18:00.7
00:41:51.84 +63:45:47.7
00:40:58.96 +64:53:57.0
00:30:16.03 +65:30:32.7
00:37:50.92 +64:51:50.1
00:32:53.14 +64:03:49.7
00:40:36.68 +63:51:02.8
00:38:49.11 +61:56:26.2
00:42:15.95 +60:40:52.7
00:31:03.31 +65:40:09.8
00:43:02.96 +63:44:54.8
00:38:28.77 +62:18:21.9
00:40:50.30 +65:22:29.8
02:33:32.98 +57:32:55.4
00:41:10.21 +60:52:06.8
00:35:51.26 +62:51:44.3
00:39:40.03 +65:15:11.8
00:41:16.70 +65:57:56.0
00:33:56.56 +64:29:16.2
00:35:38.90 +62:57:03.6
00:43:21.34 +64:17:02.3
00:36:07.37 +63:18:57.4
00:36:58.76 +63:27:39.3
00:32:19.67 +64:34:53.0
00:39:32.86 +63:41:01.9
00:39:46.41 +63:06:41.6
00:41:55.23 +59:49:28.4
00:42:50.41 +59:11:09.9
00:45:52.94 +58:02:26.8
00:48:53.39 +57:19:48.3
00:44:58.70 +57:38:27.8
00:44:56.01 +57:27:20.6
00:46:21.51 +57:49:52.5
00:50:29.28 +57:18:27.1
00:50:06.91 +57:10:27.0
00:48:55.25 +57:01:37.6
00:45:37.40 +57:38:02.0
00:46:29.05 +57:50:01.9
00:34:29.21 +64:32:50.6
00:44:24.71 +58:01:00.6
00:47:47.72 +57:43:14.4
00:45:48.57 +56:44:52.2
00:45:39.74 +56:58:20.4
00:51:36.62 +62:56:22.1
01:43:53.24 +61:53:18.3
00:50:31.14 +56:57:51.3
00:32:56.84 +66:00:52.0
02:44:30.77 +65:04:14.5
01:33:06.05 +65:23:55.5
02:44:44.99 +64:06:47.7
01:41:55.72 +57:32:30.8
01:55:36.82 +58:30:09.4
01:46:33.64 +58:55:29.0
01:55:51.31 +64:01:15.7
01:09:49.99 +65:08:27.6
02:18:52.15 +62:48:16.9
01:14:53.88 +63:36:45.3
00:37:01.11 +63:08:02.2
01:29:32.81 +63:18:25.8
01:45:35.78 +63:07:06.0
########### Completed Cas-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
00:35:58.92 +65:01:35.6
00:32:56.21 +65:13:04.3
00:46:12.54 +57:13:12.6
02:38:00.96 +63:01:46.6
00:46:54.08 +56:40:16.0
00:45:28.44 +57:19:14.0
00:46:55.79 +63:56:06.7
01:28:36.98 +62:16:38.8
00:54:54.27 +58:33:50.7
01:23:00.84 +64:39:24.5
02:30:27.23 +62:31:46.5
00:39:24.46 +64:30:15.8
00:37:33.55 +62:02:14.3
00:39:37.31 +66:00:20.5
00:49:24.50 +58:00:18.0
00:38:07.46 +61:40:25.8
00:42:46.79 +65:05:55.8
00:35:09.74 +66:10:21.1
00:36:44.04 +62:48:52.5
00:37:26.01 +64:50:45.9
00:40:27.59 +64:33:43.2
00:37:18.58 +64:11:56.4
00:33:03.73 +64:29:55.5
00:35:10.32 +65:28:35.7
00:37:14.10 +64:34:40.8
00:36:14.79 +64:20:13.2
00:36:56.00 +63:24:13.7
00:30:22.65 +65:18:31.4
00:37:07.51 +62:10:06.0
00:37:12.58 +65:18:00.7
00:41:51.84 +63:45:47.7
00:40:58.96 +64:53:57.0
00:30:16.03 +65:30:32.7
00:37:50.92 +64:51:50.1
00:32:53.14 +64:03:49.7
00:40:36.68 +63:51:02.8
00:38:49.11 +61:56:26.2
00:42:15.95 +60:40:52.7
00:31:03.31 +65:40:09.8
00:43:02.96 +63:44:54.8
00:38:28.77 +62:18:21.9
00:40:50.30 +65:22:29.8
02:33:32.98 +57:32:55.4
00:41:10.21 +60:52:06.8
00:35:51.26 +62:51:44.3
00:39:40.03 +65:15:11.8
00:41:16.70 +65:57:56.0
00:33:56.56 +64:29:16.2
00:35:38.90 +62:57:03.6
00:43:21.34 +64:17:02.3
00:36:07.37 +63:18:57.4
00:36:58.76 +63:27:39.3
00:32:19.67 +64:34:53.0
00:39:32.86 +63:41:01.9
00:39:46.41 +63:06:41.6
00:41:55.23 +59:49:28.4
00:42:50.41 +59:11:09.9
00:45:52.94 +58:02:26.8
00:48:53.39 +57:19:48.3
00:44:58.70 +57:38:27.8
00:44:56.01 +57:27:20.6
00:46:21.51 +57:49:52.5
00:50:29.28 +57:18:27.1
00:50:06.91 +57:10:27.0
00:48:55.25 +57:01:37.6
00:45:37.40 +57:38:02.0
00:46:29.05 +57:50:01.9
00:34:29.21 +64:32:50.6
00:44:24.71 +58:01:00.6
00:47:47.72 +57:43:14.4
00:45:48.57 +56:44:52.2
00:45:39.74 +56:58:20.4
00:51:36.62 +62:56:22.1
01:43:53.24 +61:53:18.3
00:50:31.14 +56:57:51.3
00:32:56.84 +66:00:52.0
02:44:30.77 +65:04:14.5
01:33:06.05 +65:23:55.5
02:44:44.99 +64:06:47.7
01:41:55.72 +57:32:30.8
01:55:36.82 +58:30:09.4
01:46:33.64 +58:55:29.0
01:55:51.31 +64:01:15.7
01:14:49.78 +57:23:46.2
00:59:00.26 +59:32:05.0
00:47:23.09 +66:08:02.9
01:45:35.78 +63:07:06.0
01:29:32.81 +63:18:25.8
01:23:06.53 +66:51:38.1
00:49:44.62 +56:57:26.4
01:25:02.46 +61:04:42.9
00:46:13.29 +57:26:24.2
02:45:28.04 +64:13:14.1
02:32:45.91 +56:29:31.8
00:42:24.91 +59:07:07.8
00:53:52.68 +57:38:01.2
01:09:49.99 +65:08:27.6
00:59:46.89 +57:17:51.8
00:46:18.28 +59:37:43.7
00:37:01.11 +63:08:02.2
00:47:14.75 +57:40:32.2
02:18:52.15 +62:48:16.9
00:43:47.49 +58:17:15.9
00:43:45.71 +58:00:44.2
01:12:11.36 +59:57:30.0
00:43:08.62 +58:24:43.2
00:48:26.10 +57:03:00.7
00:53:33.87 +57:49:00.1
02:01:09.58 +61:03:41.6
01:05:28.21 +65:58:56.5
00:54:20.03 +57:41:48.8
01:14:53.88 +63:36:45.3
###################################################################################
00:35:58.92 +65:01:35.6 -- not an asteroid (will add it to exclusion list)
00:32:56.21 +65:13:04.3 -- not an asteroid (will add it to exclusion list)
00:46:12.54 +57:13:12.6 -- not an asteroid (will add it to exclusion list)
02:38:00.96 +63:01:46.6 -- not an asteroid (will add it to exclusion list)
00:46:54.08 +56:40:16.0 -- not an asteroid (will add it to exclusion list)
00:45:28.44 +57:19:14.0 -- not an asteroid (will add it to exclusion list)
00:46:55.79 +63:56:06.7 -- not an asteroid (will add it to exclusion list)
01:28:36.98 +62:16:38.8 -- not an asteroid (will add it to exclusion list)
00:54:54.27 +58:33:50.7 -- not an asteroid (will add it to exclusion list)
01:23:00.84 +64:39:24.5 -- not an asteroid (will add it to exclusion list)
02:30:27.23 +62:31:46.5 -- not an asteroid (will add it to exclusion list)
00:39:24.46 +64:30:15.8 -- not an asteroid (will add it to exclusion list)
00:37:33.55 +62:02:14.3 -- not an asteroid (will add it to exclusion list)
00:39:37.31 +66:00:20.5 -- not an asteroid (will add it to exclusion list)
00:49:24.50 +58:00:18.0 -- not an asteroid (will add it to exclusion list)
00:38:07.46 +61:40:25.8 -- not an asteroid (will add it to exclusion list)
00:42:46.79 +65:05:55.8 -- not an asteroid (will add it to exclusion list)
00:35:09.74 +66:10:21.1 -- not an asteroid (will add it to exclusion list)
00:36:44.04 +62:48:52.5 -- not an asteroid (will add it to exclusion list)
00:37:26.01 +64:50:45.9 -- not an asteroid (will add it to exclusion list)
00:40:27.59 +64:33:43.2 -- not an asteroid (will add it to exclusion list)
00:37:18.58 +64:11:56.4 -- not an asteroid (will add it to exclusion list)
00:33:03.73 +64:29:55.5 -- not an asteroid (will add it to exclusion list)
00:35:10.32 +65:28:35.7 -- not an asteroid (will add it to exclusion list)
00:37:14.10 +64:34:40.8 -- not an asteroid (will add it to exclusion list)
00:36:14.79 +64:20:13.2 -- not an asteroid (will add it to exclusion list)
00:36:56.00 +63:24:13.7 -- not an asteroid (will add it to exclusion list)
00:30:22.65 +65:18:31.4 -- not an asteroid (will add it to exclusion list)
00:37:07.51 +62:10:06.0 -- not an asteroid (will add it to exclusion list)
00:37:12.58 +65:18:00.7 -- not an asteroid (will add it to exclusion list)
00:41:51.84 +63:45:47.7 -- not an asteroid (will add it to exclusion list)
00:40:58.96 +64:53:57.0 -- not an asteroid (will add it to exclusion list)
00:30:16.03 +65:30:32.7 -- not an asteroid (will add it to exclusion list)
00:37:50.92 +64:51:50.1 -- not an asteroid (will add it to exclusion list)
00:32:53.14 +64:03:49.7 -- not an asteroid (will add it to exclusion list)
00:40:36.68 +63:51:02.8 -- not an asteroid (will add it to exclusion list)
00:38:49.11 +61:56:26.2 -- not an asteroid (will add it to exclusion list)
00:42:15.95 +60:40:52.7 -- not an asteroid (will add it to exclusion list)
00:31:03.31 +65:40:09.8 -- not an asteroid (will add it to exclusion list)
00:43:02.96 +63:44:54.8 -- not an asteroid (will add it to exclusion list)
00:38:28.77 +62:18:21.9 -- not an asteroid (will add it to exclusion list)
00:40:50.30 +65:22:29.8 -- not an asteroid (will add it to exclusion list)
02:33:32.98 +57:32:55.4 -- not an asteroid (will add it to exclusion list)
00:41:10.21 +60:52:06.8 -- not an asteroid (will add it to exclusion list)
00:35:51.26 +62:51:44.3 -- not an asteroid (will add it to exclusion list)
00:39:40.03 +65:15:11.8 -- not an asteroid (will add it to exclusion list)
00:41:16.70 +65:57:56.0 -- not an asteroid (will add it to exclusion list)
00:33:56.56 +64:29:16.2 -- not an asteroid (will add it to exclusion list)
00:35:38.90 +62:57:03.6 -- not an asteroid (will add it to exclusion list)
00:43:21.34 +64:17:02.3 -- not an asteroid (will add it to exclusion list)
00:36:07.37 +63:18:57.4 -- not an asteroid (will add it to exclusion list)
00:36:58.76 +63:27:39.3 -- not an asteroid (will add it to exclusion list)
00:32:19.67 +64:34:53.0 -- not an asteroid (will add it to exclusion list)
00:39:32.86 +63:41:01.9 -- not an asteroid (will add it to exclusion list)
00:39:46.41 +63:06:41.6 -- not an asteroid (will add it to exclusion list)
00:41:55.23 +59:49:28.4 -- not an asteroid (will add it to exclusion list)
00:42:50.41 +59:11:09.9 -- not an asteroid (will add it to exclusion list)
00:45:52.94 +58:02:26.8 -- not an asteroid (will add it to exclusion list)
00:48:53.39 +57:19:48.3 -- not an asteroid (will add it to exclusion list)
00:44:58.70 +57:38:27.8 -- not an asteroid (will add it to exclusion list)
00:44:56.01 +57:27:20.6 -- not an asteroid (will add it to exclusion list)
00:46:21.51 +57:49:52.5 -- not an asteroid (will add it to exclusion list)
00:50:29.28 +57:18:27.1 -- not an asteroid (will add it to exclusion list)
00:50:06.91 +57:10:27.0 -- not an asteroid (will add it to exclusion list)
00:48:55.25 +57:01:37.6 -- not an asteroid (will add it to exclusion list)
00:45:37.40 +57:38:02.0 -- not an asteroid (will add it to exclusion list)
00:46:29.05 +57:50:01.9 -- not an asteroid (will add it to exclusion list)
00:34:29.21 +64:32:50.6 -- not an asteroid (will add it to exclusion list)
00:44:24.71 +58:01:00.6 -- not an asteroid (will add it to exclusion list)
00:47:47.72 +57:43:14.4 -- not an asteroid (will add it to exclusion list)
00:45:48.57 +56:44:52.2 -- not an asteroid (will add it to exclusion list)
00:45:39.74 +56:58:20.4 -- not an asteroid (will add it to exclusion list)
00:51:36.62 +62:56:22.1 -- not an asteroid (will add it to exclusion list)
01:43:53.24 +61:53:18.3 -- not an asteroid (will add it to exclusion list)
00:50:31.14 +56:57:51.3 -- not an asteroid (will add it to exclusion list)
00:32:56.84 +66:00:52.0 -- not an asteroid (will add it to exclusion list)
02:44:30.77 +65:04:14.5 -- not an asteroid (will add it to exclusion list)
01:33:06.05 +65:23:55.5 -- not an asteroid (will add it to exclusion list)
02:44:44.99 +64:06:47.7 -- not an asteroid (will add it to exclusion list)
01:41:55.72 +57:32:30.8 -- not an asteroid (will add it to exclusion list)
01:55:36.82 +58:30:09.4 -- not an asteroid (will add it to exclusion list)
01:46:33.64 +58:55:29.0 -- not an asteroid (will add it to exclusion list)
01:55:51.31 +64:01:15.7 -- not an asteroid (will add it to exclusion list)
01:14:49.78 +57:23:46.2 -- not an asteroid (will add it to exclusion list)
00:59:00.26 +59:32:05.0 -- not an asteroid (will add it to exclusion list)
00:47:23.09 +66:08:02.9 -- not an asteroid (will add it to exclusion list)
01:45:35.78 +63:07:06.0 -- not an asteroid (will add it to exclusion list)
01:29:32.81 +63:18:25.8 -- not an asteroid (will add it to exclusion list)
01:23:06.53 +66:51:38.1 -- not an asteroid (will add it to exclusion list)
00:49:44.62 +56:57:26.4 -- not an asteroid (will add it to exclusion list)
01:25:02.46 +61:04:42.9 -- not an asteroid (will add it to exclusion list)
00:46:13.29 +57:26:24.2 -- not an asteroid (will add it to exclusion list)
02:45:28.04 +64:13:14.1 -- not an asteroid (will add it to exclusion list)
02:32:45.91 +56:29:31.8 -- not an asteroid (will add it to exclusion list)
00:42:24.91 +59:07:07.8 -- not an asteroid (will add it to exclusion list)
00:53:52.68 +57:38:01.2 -- not an asteroid (will add it to exclusion list)
01:09:49.99 +65:08:27.6 -- not an asteroid (will add it to exclusion list)
00:59:46.89 +57:17:51.8 -- not an asteroid (will add it to exclusion list)
00:46:18.28 +59:37:43.7 -- not an asteroid (will add it to exclusion list)
00:37:01.11 +63:08:02.2 -- not an asteroid (will add it to exclusion list)
00:47:14.75 +57:40:32.2 -- not an asteroid (will add it to exclusion list)
02:18:52.15 +62:48:16.9 -- not an asteroid (will add it to exclusion list)
00:43:47.49 +58:17:15.9 -- not an asteroid (will add it to exclusion list)
00:43:45.71 +58:00:44.2 -- not an asteroid (will add it to exclusion list)
01:12:11.36 +59:57:30.0 -- not an asteroid (will add it to exclusion list)
00:43:08.62 +58:24:43.2 -- not an asteroid (will add it to exclusion list)
00:48:26.10 +57:03:00.7 -- not an asteroid (will add it to exclusion list)
00:53:33.87 +57:49:00.1 -- not an asteroid (will add it to exclusion list)
02:01:09.58 +61:03:41.6 -- not an asteroid (will add it to exclusion list)
01:05:28.21 +65:58:56.5 -- not an asteroid (will add it to exclusion list)
00:54:20.03 +57:41:48.8 -- not an asteroid (will add it to exclusion list)
01:14:53.88 +63:36:45.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:30:16.03 +65:30:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:22.65 +65:18:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:03.31 +65:40:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:19.67 +64:34:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:53.14 +64:03:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:56.21 +65:13:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:56.84 +66:00:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:03.73 +64:29:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:56.56 +64:29:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:29.21 +64:32:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:09.74 +66:10:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:10.32 +65:28:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:38.90 +62:57:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:51.26 +62:51:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:58.92 +65:01:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:07.37 +63:18:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:14.79 +64:20:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:44.04 +62:48:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:56.00 +63:24:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:58.76 +63:27:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:01.11 +63:08:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:07.51 +62:10:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:12.58 +65:18:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:14.10 +64:34:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:18.58 +64:11:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:26.01 +64:50:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:33.55 +62:02:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:50.92 +64:51:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:07.46 +61:40:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:28.77 +62:18:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:49.11 +61:56:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:24.46 +64:30:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:32.86 +63:41:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:37.31 +66:00:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:40.03 +65:15:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:46.41 +63:06:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:27.59 +64:33:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:36.68 +63:51:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:50.30 +65:22:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:58.96 +64:53:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:10.21 +60:52:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:16.70 +65:57:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:51.84 +63:45:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:55.23 +59:49:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:15.95 +60:40:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:24.91 +59:07:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:46.79 +65:05:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:50.41 +59:11:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:02.96 +63:44:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:08.62 +58:24:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:21.34 +64:17:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:45.71 +58:00:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:47.49 +58:17:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:24.71 +58:01:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:56.01 +57:27:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:58.70 +57:38:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:28.44 +57:19:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:37.40 +57:38:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:39.74 +56:58:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:48.57 +56:44:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:52.94 +58:02:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:12.54 +57:13:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:13.29 +57:26:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:18.28 +59:37:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:21.51 +57:49:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:29.05 +57:50:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:54.08 +56:40:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:55.79 +63:56:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:14.75 +57:40:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:23.09 +66:08:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:47.72 +57:43:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:26.10 +57:03:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:53.39 +57:19:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:55.25 +57:01:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:24.50 +58:00:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:44.62 +56:57:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:06.91 +57:10:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:29.28 +57:18:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:31.14 +56:57:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:36.62 +62:56:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:33.87 +57:49:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:52.68 +57:38:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:20.03 +57:41:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:54.27 +58:33:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:00.26 +59:32:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:46.89 +57:17:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:28.21 +65:58:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:49.99 +65:08:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:11.36 +59:57:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:49.78 +57:23:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:53.88 +63:36:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:00.84 +64:39:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:06.53 +66:51:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:02.46 +61:04:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:36.98 +62:16:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:32.81 +63:18:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:06.05 +65:23:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:55.72 +57:32:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:53.24 +61:53:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:35.78 +63:07:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:33.64 +58:55:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:36.82 +58:30:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:51.31 +64:01:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:09.58 +61:03:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:52.15 +62:48:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:27.23 +62:31:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:45.91 +56:29:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:32.98 +57:32:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:00.96 +63:01:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:44:30.77 +65:04:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:44:44.99 +64:06:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:45:28.04 +64:13:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:30:16.03 +65:30:32.7 -- not a known variable star
00:30:22.65 +65:18:31.4 -- not a known variable star
00:31:03.31 +65:40:09.8 -- not a known variable star
00:32:19.67 +64:34:53.0 -- not a known variable star
00:32:53.14 +64:03:49.7 -- not a known variable star
00:32:56.21 +65:13:04.3 -- not a known variable star
00:32:56.84 +66:00:52.0 -- not a known variable star
00:33:03.73 +64:29:55.5 -- not a known variable star
00:33:56.56 +64:29:16.2 -- not a known variable star
00:34:29.21 +64:32:50.6 -- a known variable star
00:35:09.74 +66:10:21.1 -- not a known variable star
00:35:10.32 +65:28:35.7 -- not a known variable star
00:35:38.90 +62:57:03.6 -- not a known variable star
00:35:51.26 +62:51:44.3 -- not a known variable star
00:35:58.92 +65:01:35.6 -- a known variable star
00:36:07.37 +63:18:57.4 -- not a known variable star
00:36:14.79 +64:20:13.2 -- not a known variable star
00:36:44.04 +62:48:52.5 -- a known variable star
00:36:56.00 +63:24:13.7 -- a known variable star
00:36:58.76 +63:27:39.3 -- not a known variable star
00:37:01.11 +63:08:02.2 -- a known variable star
00:37:07.51 +62:10:06.0 -- not a known variable star
00:37:12.58 +65:18:00.7 -- a known variable star
00:37:14.10 +64:34:40.8 -- not a known variable star
00:37:18.58 +64:11:56.4 -- not a known variable star
00:37:26.01 +64:50:45.9 -- not a known variable star
00:37:33.55 +62:02:14.3 -- not a known variable star
00:37:50.92 +64:51:50.1 -- not a known variable star
00:38:07.46 +61:40:25.8 -- not a known variable star
00:38:28.77 +62:18:21.9 -- not a known variable star
00:38:49.11 +61:56:26.2 -- a known variable star
00:39:24.46 +64:30:15.8 -- not a known variable star
00:39:32.86 +63:41:01.9 -- a known variable star
00:39:37.31 +66:00:20.5 -- a known variable star
00:39:40.03 +65:15:11.8 -- not a known variable star
00:39:46.41 +63:06:41.6 -- not a known variable star
00:40:27.59 +64:33:43.2 -- not a known variable star
00:40:36.68 +63:51:02.8 -- not a known variable star
00:40:50.30 +65:22:29.8 -- not a known variable star
00:40:58.96 +64:53:57.0 -- not a known variable star
00:41:10.21 +60:52:06.8 -- a known variable star
00:41:16.70 +65:57:56.0 -- a known variable star
00:41:51.84 +63:45:47.7 -- not a known variable star
00:41:55.23 +59:49:28.4 -- not a known variable star
00:42:15.95 +60:40:52.7 -- a known variable star
00:42:24.91 +59:07:07.8 -- a known variable star
00:42:46.79 +65:05:55.8 -- a known variable star
00:42:50.41 +59:11:09.9 -- not a known variable star
00:43:02.96 +63:44:54.8 -- not a known variable star
00:43:08.62 +58:24:43.2 -- not a known variable star
00:43:21.34 +64:17:02.3 -- not a known variable star
00:43:45.71 +58:00:44.2 -- a known variable star
00:43:47.49 +58:17:15.9 -- not a known variable star
00:44:24.71 +58:01:00.6 -- not a known variable star
00:44:56.01 +57:27:20.6 -- not a known variable star
00:44:58.70 +57:38:27.8 -- not a known variable star
00:45:28.44 +57:19:14.0 -- a known variable star
00:45:37.40 +57:38:02.0 -- not a known variable star
00:45:39.74 +56:58:20.4 -- not a known variable star
00:45:48.57 +56:44:52.2 -- not a known variable star
00:45:52.94 +58:02:26.8 -- not a known variable star
00:46:12.54 +57:13:12.6 -- a known variable star
00:46:13.29 +57:26:24.2 -- a known variable star
00:46:18.28 +59:37:43.7 -- a known variable star
00:46:21.51 +57:49:52.5 -- not a known variable star
00:46:29.05 +57:50:01.9 -- a known variable star
00:46:54.08 +56:40:16.0 -- a known variable star
00:46:55.79 +63:56:06.7 -- a known variable star
00:47:14.75 +57:40:32.2 -- a known variable star
00:47:23.09 +66:08:02.9 -- a known variable star
00:47:47.72 +57:43:14.4 -- a known variable star
00:48:26.10 +57:03:00.7 -- not a known variable star
00:48:53.39 +57:19:48.3 -- not a known variable star
00:48:55.25 +57:01:37.6 -- not a known variable star
00:49:24.50 +58:00:18.0 -- not a known variable star
00:49:44.62 +56:57:26.4 -- not a known variable star
00:50:06.91 +57:10:27.0 -- a known variable star
00:50:29.28 +57:18:27.1 -- a known variable star
00:50:31.14 +56:57:51.3 -- a known variable star
00:51:36.62 +62:56:22.1 -- not a known variable star
00:53:33.87 +57:49:00.1 -- a known variable star
00:53:52.68 +57:38:01.2 -- not a known variable star
00:54:20.03 +57:41:48.8 -- not a known variable star
00:54:54.27 +58:33:50.7 -- a known variable star
00:59:00.26 +59:32:05.0 -- not a known variable star
00:59:46.89 +57:17:51.8 -- not a known variable star
01:05:28.21 +65:58:56.5 -- a known variable star
01:09:49.99 +65:08:27.6 -- a known variable star
01:12:11.36 +59:57:30.0 -- a known variable star
01:14:49.78 +57:23:46.2 -- a known variable star
01:14:53.88 +63:36:45.3 -- a known variable star
01:23:00.84 +64:39:24.5 -- a known variable star
01:23:06.53 +66:51:38.1 -- not a known variable star
01:25:02.46 +61:04:42.9 -- a known variable star
01:28:36.98 +62:16:38.8 -- a known variable star
01:29:32.81 +63:18:25.8 -- not a known variable star
01:33:06.05 +65:23:55.5 -- not a known variable star
01:41:55.72 +57:32:30.8 -- not a known variable star
01:43:53.24 +61:53:18.3 -- a known variable star
01:45:35.78 +63:07:06.0 -- a known variable star
01:46:33.64 +58:55:29.0 -- not a known variable star
01:55:36.82 +58:30:09.4 -- not a known variable star
01:55:51.31 +64:01:15.7 -- not a known variable star
02:01:09.58 +61:03:41.6 -- a known variable star
02:18:52.15 +62:48:16.9 -- a known variable star
02:30:27.23 +62:31:46.5 -- a known variable star
02:32:45.91 +56:29:31.8 -- a known variable star
02:33:32.98 +57:32:55.4 -- a known variable star
02:38:00.96 +63:01:46.6 -- a known variable star
02:44:30.77 +65:04:14.5 -- not a known variable star
02:44:44.99 +64:06:47.7 -- a known variable star
02:45:28.04 +64:13:14.1 -- not a known variable star
Found 65 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
112 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 112 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461119.57859100 -observatory 500
22:37:26.83 -07:25:46.8 Mercury (1.2mag)
01:02:23.06 +05:41:04.8 Venus (-3.9mag)
23:00:28.52 -07:31:09.6 Mars (1.2mag)
07:04:38.51 +22:58:09.2 Jupiter (-2.3mag)
00:16:55.64 -00:28:54.1 Saturn (0.9mag)
03:42:47.85 +19:31:24.6 Uranus (5.8mag)
00:07:09.70 -00:38:51.8 Neptune (7.8mag)
20:31:55.35 -22:53:55.3 Pluto (14.5mag)
00:41:18.51 +07:37:36.9 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Mar 19 21:20 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461119.57859100:
07:04:29.51 +22:58:25.6 Io (5.6mag)
07:04:41.73 +22:57:59.4 Europa (5.7mag)
07:04:29.35 +22:58:18.6 Ganymede (5.2mag)
07:04:10.14 +22:58:53.4 Callisto (6.4mag)
07:08:39.95 +23:00:18.4 Himalia (15.2mag)
07:04:37.96 +22:58:07.3 Thebe (16.0mag)
07:08:13.70 +23:23:10.4 Elara (17.1mag)
07:01:42.94 +23:52:19.6 Pasiphae (17.2mag)
07:13:26.68 +22:52:26.4 Carme (18.3mag)
00:16:47.38 -00:28:43.0 Titan (8.8mag)
00:16:54.74 -00:28:48.5 Rhea (10.1mag)
00:17:26.07 -00:26:55.8 Iapetus (11.5mag)
00:17:09.70 -00:29:02.6 Hyperion (14.8mag)
00:18:50.26 -00:17:33.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 19 21:20 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461119.57859100:
12:42:08.40 +09:49:34.8 JWST
19:17:59.79 +13:28:07.0 Chandra
15:16:28.29 -59:57:07.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 19 21:20 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461119.57859100 -observatory 500
18:34:37.51 -27:25:16.0 14.1mag P/2010 H2 (Vales)
04:50:44.37 -71:05:10.0 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:40.80 +31:17:40.8 17.0mag C/2017 K2 (PANSTARRS)
17:29:28.85 +07:17:39.6 17.6mag C/2021 G2 (ATLAS)
23:01:11.81 +28:25:06.9 16.9mag C/2022 E2 (ATLAS)
03:59:32.70 +25:16:03.8 15.7mag C/2022 N2 (PANSTARRS)
09:01:58.92 +31:24:42.9 16.0mag C/2022 QE78 (ATLAS)
08:30:16.67 -03:17:31.9 17.2mag C/2022 R6 (PANSTARRS)
18:56:28.23 +16:12:46.2 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:26.75 -11:51:13.8 17.6mag P/2023 B1 (PANSTARRS)
09:25:18.39 -16:29:25.5 17.4mag C/2023 F3 (ATLAS)
21:20:18.71 +61:39:59.6 17.4mag C/2023 H5 (Lemmon)
19:33:25.70 -03:31:03.6 14.5mag C/2023 R1 (PANSTARRS)
21:35:33.54 +82:46:19.8 17.7mag C/2023 X2 (Lemmon)
06:15:43.07 +63:47:54.7 16.8mag C/2024 A1 (ATLAS)
04:03:25.04 +04:30:32.6 9.0mag C/2024 E1 (Wierzchos)
11:23:24.17 +02:32:53.3 18.0mag C/2024 G2 (ATLAS)
16:32:35.43 +02:01:13.5 17.5mag C/2024 G6 (ATLAS)
20:09:33.93 +08:33:16.8 14.9mag C/2024 J3 (ATLAS)
03:04:00.43 -26:48:55.2 16.5mag C/2024 T5 (ATLAS)
04:57:00.28 +52:54:03.1 17.6mag C/2025 J1 (Borisov)
15:16:13.97 +16:13:17.8 14.4mag C/2025 L1 (ATLAS)
02:47:22.90 -22:27:38.9 17.6mag C/2025 Q3 (ATLAS)
22:32:19.40 +18:57:06.8 12.6mag C/2025 R3 (PANSTARRS)
13:05:24.95 +01:15:03.4 17.7mag C/2025 Y1 (ATLAS)
02:12:01.96 -06:54:48.6 14.3mag C/2026 A1 (MAPS)
22:35:48.31 +30:45:49.9 13.7mag C/2026 B2 (Sun-Gao)
17:50:16.22 -10:52:01.7 13.4mag 10P/Tempel
15:27:12.97 +05:11:01.3 11.7mag 24P/Schaumasse
11:12:23.16 -02:30:59.7 15.6mag 29P/Schwassmann-Wachmann
17:42:42.45 -10:40:49.1 17.3mag 40P/Vaisala
10:45:38.42 -06:39:39.5 16.4mag 43P/Wolf-Harrington
01:07:34.37 +12:45:25.8 17.0mag 47P/Ashbrook-Jackson
06:27:21.61 +42:31:54.3 17.1mag 63P/Wild
22:52:54.17 -14:51:49.9 15.7mag 65P/Gunn
02:56:20.07 +10:56:16.6 15.9mag 76P/West-Kohoutek-Ikemura
00:07:34.70 +02:51:54.5 14.7mag 78P/Gehrels
21:35:33.47 -16:58:47.8 14.5mag 88P/Howell
00:58:26.16 +12:57:06.8 15.3mag 93P/Lovas
04:09:13.54 +30:37:24.8 16.5mag 123P/West-Hartley
08:07:33.05 +50:40:31.6 16.2mag 124P/Mrkos
01:53:00.74 +11:14:40.0 16.4mag 128P/Shoemaker-Holt
01:55:39.47 +10:54:05.0 17.4mag 131P/Mueller
23:16:03.99 +02:43:50.6 13.1mag 141P/Machholz
23:26:07.93 -04:43:28.3 13.1mag 141P-A/Machholz
22:27:28.91 -07:12:14.1 16.2mag 141P-D/Machholz
23:47:51.06 -14:34:14.3 15.5mag 162P/SidingSpring
10:40:00.12 +32:02:14.7 17.5mag 164P/Christensen
05:48:09.18 +24:44:28.9 17.5mag 198P/ODAS
15:34:30.74 -03:30:01.2 16.9mag 210P/Christensen
20:08:17.32 -17:44:29.4 17.1mag 218P/LINEAR
16:58:17.14 -16:45:14.9 16.3mag 235P/LINEAR
04:39:41.99 +31:52:38.0 16.3mag 240P/NEAT
07:29:44.74 -08:29:57.4 17.5mag 242P/Spahr
15:48:37.02 +05:02:08.4 17.7mag 391P/Kowalski
07:27:55.35 +21:05:29.8 17.5mag 450P/LONEOS
04:59:51.24 +46:40:39.6 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 19 21:20 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
-rw-r--r-- 1 apache apache 5.7K Mar 19 21:20 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 19 21:20 tocp_transients_list.txt
