This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm
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 02 27.1856* 02 19 14.40 +51 15 28.2 10.2 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
BV Per,2461098.6857,10.19,0.05,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
BV Per 20260227.1857 10.19CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:19:14.40 +51:15:28.2 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 56 32.09 +57 23 06.0 14.1 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 505338430345408896,2461098.6857,14.12,0.05,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
Gaia DR3 505338430345408896 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:56:32.09 +57:23:06.0 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.59 02:03:22.79 +49:39:05.0
134.70629 -11.56855 galactic Per Second-epoch detections are separated by 4.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 358352589206844160 | 02:03:23.10 +49:39:11.2 (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 02 27.1856* 02 03 22.79 +49 39 05.0 13.6 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 358352589206844160,2461098.6857,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 358352589206844160 20260227.1857 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:22.79 +49:39:05.0 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.54 01:59:11.99 +51:55:30.9
133.43102 -9.55979 galactic Per Second-epoch detections are separated by 2.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 359629538822658688 | 01:59:12.66 +51:55:33.6 (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 02 27.1856* 01 59 11.99 +51 55 30.9 13.5 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 359629538822658688,2461098.6857,13.54,0.05,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 359629538822658688 20260227.1857 13.54CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:59:11.99 +51:55:30.9 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.48 02:03:54.56 +49:11:54.6
134.92101 -11.97884 galactic Per Second-epoch detections are separated by 5.2" and 4.4 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 J030.9810+49.1994 | 02:03:55.44 +49:11:58.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1856* 02 03 54.56 +49 11 54.6 13.5 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
ATO J030.9810+49.1994,2461098.6857,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J030.9810+49.1994 20260227.1857 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:54.56 +49:11:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.64 02:01:45.17 +58:24:19.7
132.05043 -3.21592 galactic Cas Second-epoch detections are separated by 2.6" and 3.1 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 505503769406850432 | 02:01:43.60 +58:24:20.3 (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 02 27.1856* 02 01 45.17 +58 24 19.7 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
Gaia DR3 505503769406850432,2461098.6857,13.64,0.05,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 505503769406850432 20260227.1857 13.64CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:01:45.17 +58:24:19.7 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1972556,2461098.6857,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1972556 20260227.1857 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:50.82 +56:50:37.1 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 57 48.22 +57 18 36.4 13.5 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
ASASSN-V J015746.90+571834.4,2461098.6857,13.54,0.05,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 J015746.90+571834.4 20260227.1857 13.54CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:57:48.22 +57:18:36.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.46 01:54:31.93 +56:47:31.8
131.52712 -5.02296 galactic Per Second-epoch detections are separated by 4.7" 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 | ATO J028.6352+56.7886 | 01:54:30.13 +56:47:30.3 (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 02 27.1856* 01 54 31.93 +56 47 31.8 13.5 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
ATO J028.6352+56.7886,2461098.6857,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J028.6352+56.7886 20260227.1857 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:54:31.93 +56:47:31.8 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 53 33.90 +57 43 27.6 13.5 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 506111941077672192,2461098.6857,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506111941077672192 20260227.1857 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:53:33.90 +57:43:27.6 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.36 01:57:17.91 +56:32:02.5
131.96106 -5.17874 galactic Per Second-epoch detections are separated by 6.9" 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 504878976227787264 | 01:57:17.07 +56:32:03.2 (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 02 27.1856* 01 57 17.91 +56 32 02.5 13.4 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 504878976227787264,2461098.6857,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 504878976227787264 20260227.1857 13.36CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:57:17.91 +56:32:02.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 54 22.12 +57 13 18.8 13.3 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 504963363741774464,2461098.6857,13.35,0.05,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 504963363741774464 20260227.1857 13.35CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:54:22.12 +57:13:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 53 50.28 +58 01 22.9 13.6 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
ZTF J015350.89+580127.1,2461098.6857,13.60,0.05,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
ZTF J015350.89+580127.1 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:53:50.28 +58:01:22.9 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.37 01:58:23.03 +55:54:35.4
132.26774 -5.74370 galactic Per Second-epoch detections are separated by 1.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J029.5918+55.9092 | 01:58:22.04 +55:54:33.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1856* 01 58 23.03 +55 54 35.4 13.4 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
ATO J029.5918+55.9092,2461098.6857,13.37,0.05,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
ATO J029.5918+55.9092 20260227.1857 13.37CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:58:23.03 +55:54:35.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.45 01:57:10.61 +57:18:12.5
131.74965 -4.43851 galactic Per Second-epoch detections are separated by 0.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J029.2982+57.3033 | 01:57:11.59 +57:18:12.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1856* 01 57 10.61 +57 18 12.5 13.4 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
ATO J029.2982+57.3033,2461098.6857,13.45,0.05,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 J029.2982+57.3033 20260227.1857 13.45CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:57:10.61 +57:18:12.5 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.35 02:01:27.67 +50:11:24.2
134.25158 -11.13636 galactic Per Second-epoch detections are separated by 2.9" and 3.5 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 358448830833843712 | 02:01:28.35 +50:11:29.1 (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 02 27.1856* 02 01 27.67 +50 11 24.2 13.3 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 358448830833843712,2461098.6857,13.35,0.05,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 358448830833843712 20260227.1857 13.35CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:01:27.67 +50:11:24.2 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.18 02:01:37.10 +58:22:38.8
132.04098 -3.24765 galactic Cas Second-epoch detections are separated by 7.4" and 1.7 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 505497756452636928 | 02:01:36.28 +58:22:39.2 (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 02 27.1856* 02 01 37.10 +58 22 38.8 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
Gaia DR3 505497756452636928,2461098.6857,13.18,0.05,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 505497756452636928 20260227.1857 13.18CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:01:37.10 +58:22:38.8 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.26 01:53:54.96 +56:44:08.9
131.45855 -5.09806 galactic Per Second-epoch detections are separated by 6.8" 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 | ATO J028.4721+56.7355 | 01:53:53.32 +56:44:08.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G1 (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 02 27.1856* 01 53 54.96 +56 44 08.9 13.3 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
ATO J028.4721+56.7355,2461098.6857,13.26,0.05,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
ATO J028.4721+56.7355 20260227.1857 13.26CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:53:54.96 +56:44:08.9 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 58 21.88 +58 00 55.1 13.4 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
ASASSN-V J015820.58+580055.7,2461098.6857,13.36,0.05,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
ASASSN-V J015820.58+580055.7 20260227.1857 13.36CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:58:21.88 +58:00:55.1 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 55 01.43 +57 05 05.8 13.1 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
ZTF J015459.89+570506.3,2461098.6857,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J015459.89+570506.3 20260227.1857 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:01.43 +57:05:05.8 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.27 02:00:44.09 +58:16:23.8
131.95690 -3.37901 galactic Cas Second-epoch detections are separated by 1.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J030.1859+58.2726 | 02:00:42.79 +58:16:27.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1856* 02 00 44.09 +58 16 23.8 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J030.1859+58.2726,2461098.6857,13.27,0.05,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 J030.1859+58.2726 20260227.1857 13.27CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:00:44.09 +58:16:23.8 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.16 02:01:26.14 +56:17:43.5
132.57821 -5.25973 galactic Per Second-epoch detections are separated by 5.2" and 2.9 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 | ZTF J020124.00+561719.3 | 02:01:25.44 +56:17:40.2 (Gaia DR3) | BY (local) | 2458432.76440 (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 02 27.1856* 02 01 26.14 +56 17 43.5 13.2 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
ZTF J020124.00+561719.3,2461098.6857,13.16,0.05,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
ZTF J020124.00+561719.3 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:01:26.14 +56:17:43.5 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 59 58.86 +57 13 28.3 13.3 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 505300364059285120,2461098.6857,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505300364059285120 20260227.1857 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:59:58.86 +57:13:28.3 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.08 01:59:37.71 +58:21:54.2
131.79231 -3.32874 galactic Cas Second-epoch detections are separated by 1.3" and 3.1 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 505488311822993536 | 01:59:38.55 +58:21:55.4 (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 02 27.1856* 01 59 37.71 +58 21 54.2 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
Large-amplitude variable Gaia DR2 505488311822993536,2461098.6857,13.08,0.05,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
Large-amplitude variable Gaia DR2 505488311822993536 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:59:37.71 +58:21:54.2 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.97 01:56:10.98 +55:30:13.3
132.06978 -6.21516 galactic Per Second-epoch detections are separated by 1.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J029.0399+55.5037 | 01:56:09.58 +55:30:13.6 (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 02 27.1856* 01 56 10.98 +55 30 13.3 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
ATO J029.0399+55.5037,2461098.6857,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J029.0399+55.5037 20260227.1857 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:56:10.98 +55:30:13.3 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.04 01:53:33.64 +58:23:36.9
131.01375 -3.50001 galactic Cas Second-epoch detections are separated by 4.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J028.3937+58.3935 | 01:53:34.50 +58:23:36.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.286 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1856* 01 53 33.64 +58 23 36.9 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
ATO J028.3937+58.3935,2461098.6857,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J028.3937+58.3935 20260227.1857 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:53:33.64 +58:23:36.9 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.09 01:55:47.67 +55:57:51.4
131.90133 -5.78266 galactic Per Second-epoch detections are separated by 4.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J028.9354+55.9603 | 01:55:46.44 +55:57:51.4 (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 02 27.1856* 01 55 47.67 +55 57 51.4 13.1 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
ATO J028.9354+55.9603,2461098.6857,13.09,0.05,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
ATO J028.9354+55.9603 20260227.1857 13.09CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:47.67 +55:57:51.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 58 39.94 +58 15 34.9 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
Gaia DR3 505486525123485696,2461098.6857,13.10,0.05,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 505486525123485696 20260227.1857 13.10CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:58:39.94 +58:15:34.9 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.10 01:57:25.67 +55:41:39.6
132.19263 -5.98639 galactic Per Second-epoch detections are separated by 3.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J029.3516+55.6940 | 01:57:24.39 +55:41:38.5 (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 02 27.1856* 01 57 25.67 +55 41 39.6 13.1 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
ATO J029.3516+55.6940,2461098.6857,13.10,0.05,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
ATO J029.3516+55.6940 20260227.1857 13.10CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:57:25.67 +55:41:39.6 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.07 01:56:42.84 +57:03:00.6
131.75272 -4.69945 galactic Per Second-epoch detections are separated by 3.8" and 3.2 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 504943641257068800 | 01:56:41.71 +57:02:59.3 (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 02 27.1856* 01 56 42.84 +57 03 00.6 13.1 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 504943641257068800,2461098.6857,13.07,0.05,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
Gaia DR3 504943641257068800 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:56:42.84 +57:03:00.6 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.97 01:57:31.19 +58:04:39.1
131.59771 -3.67806 galactic Per Second-epoch detections are separated by 6.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J029.3902+58.0783 | 01:57:32.16 +58:04:37.3 (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 02 27.1856* 01 57 31.19 +58 04 39.1 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
ATO J029.3902+58.0783,2461098.6857,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J029.3902+58.0783 20260227.1857 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:57:31.19 +58:04:39.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.94 02:01:39.48 +51:08:45.5
134.01675 -10.20819 galactic Per Second-epoch detections are separated by 2.3" and 3.8 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 | ATO J030.4178+51.1494 | 02:01:40.16 +51:08:45.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (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 02 27.1856* 02 01 39.48 +51 08 45.5 12.9 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
ATO J030.4178+51.1494,2461098.6857,12.94,0.05,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
ATO J030.4178+51.1494 20260227.1857 12.94CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:01:39.48 +51:08:45.5 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.02 01:53:17.83 +57:14:43.9
131.25399 -4.62332 galactic Per Second-epoch detections are separated by 1.9" and 2.9 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 505708897044808320 | 01:53:15.44 +57:14:31.7 (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 02 27.1856* 01 53 17.83 +57 14 43.9 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
Gaia DR3 505708897044808320,2461098.6857,13.02,0.05,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
Gaia DR3 505708897044808320 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:53:17.83 +57:14:43.9 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.90 02:00:30.82 +58:23:14.7
131.89855 -3.27665 galactic Cas Second-epoch detections are separated by 1.6" and 3.2 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 505500131581074560 | 02:00:31.74 +58:23:14.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.964+/- (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 02 27.1856* 02 00 30.82 +58 23 14.7 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 505500131581074560,2461098.6857,12.90,0.05,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 505500131581074560 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:00:30.82 +58:23:14.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.88 01:58:23.60 +58:14:23.2
131.66784 -3.49178 galactic Cas Second-epoch detections are separated by 4.5" and 2.6 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 J029.5953+58.2384 | 01:58:22.36 +58:14:24.4 (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 02 27.1856* 01 58 23.60 +58 14 23.2 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J029.5953+58.2384,2461098.6857,12.88,0.05,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
ATO J029.5953+58.2384 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:58:23.60 +58:14:23.2 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.88 02:02:29.09 +57:55:02.1
132.27590 -3.65979 galactic Per Second-epoch detections are separated by 2.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J030.6250+57.9171 | 02:02:28.20 +57:54:59.7 (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 02 27.1856* 02 02 29.09 +57 55 02.1 12.9 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
ATO J030.6250+57.9171,2461098.6857,12.88,0.05,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
ATO J030.6250+57.9171 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:02:29.09 +57:55:02.1 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.70 01:54:45.11 +57:29:50.1
131.38410 -4.33179 galactic Per Second-epoch detections are separated by 5.1" and 2.3 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 | Large-amplitude variable Gaia DR2 506092802703581952 | 01:54:43.80 +57:29:50.8 (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 02 27.1856* 01 54 45.11 +57 29 50.1 12.7 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
Large-amplitude variable Gaia DR2 506092802703581952,2461098.6857,12.70,0.05,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
Large-amplitude variable Gaia DR2 506092802703581952 20260227.1857 12.70CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:54:45.11 +57:29:50.1 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.76 01:55:49.17 +57:55:52.4
131.41591 -3.87611 galactic Per Second-epoch detections are separated by 4.0" and 3.2 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 506130495337496320 | 01:55:47.77 +57:55:53.1 (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 02 27.1856* 01 55 49.17 +57 55 52.4 12.8 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 506130495337496320,2461098.6857,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506130495337496320 20260227.1857 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:49.17 +57:55:52.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 58 32.91 +56 30 56.7 12.4 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 504867740593547264,2461098.6857,12.38,0.05,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 504867740593547264 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:58:32.91 +56:30:56.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.39 01:55:08.51 +56:58:20.0
131.56409 -4.82803 galactic Per Second-epoch detections are separated by 2.0" and 2.9 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 504951269118838400 | 01:55:07.06 +56:58:21.7 (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 02 27.1856* 01 55 08.51 +56 58 20.0 12.4 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 504951269118838400,2461098.6857,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 504951269118838400 20260227.1857 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:08.51 +56:58:20.0 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.24 01:59:54.17 +57:34:41.1
132.03409 -4.07870 galactic Per Second-epoch detections are separated by 0.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 505314382832177280 | 01:59:55.01 +57:34:40.8 (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 02 27.1856* 01 59 54.17 +57 34 41.1 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 505314382832177280,2461098.6857,12.24,0.05,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 505314382832177280 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:59:54.17 +57:34:41.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.21 01:56:28.02 +58:12:14.2
131.43111 -3.59066 galactic Cas Second-epoch detections are separated by 3.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506140184783427840 | 01:56:26.72 +58:12:16.0 (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 02 27.1856* 01 56 28.02 +58 12 14.2 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
Gaia DR3 506140184783427840,2461098.6857,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506140184783427840 20260227.1857 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:56:28.02 +58:12:14.2 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 54 13.49 +57 32 11.1 12.1 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 506093970934672512,2461098.6857,12.12,0.05,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
Gaia DR3 506093970934672512 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:54:13.49 +57:32:11.1 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 11.73 01:53:46.47 +57:10:59.6
131.33188 -4.66838 galactic Per Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J028.4334+57.1905 | 01:53:44.22 +57:11:01.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8III 1928MeUpp..37....1S BD+56 380
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 02 27.1856* 01 53 46.47 +57 10 59.6 11.7 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
ATO J028.4334+57.1905,2461098.6857,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J028.4334+57.1905 20260227.1857 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:53:46.47 +57:10:59.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 11.32 01:57:01.66 +56:14:15.7
131.99989 -5.47492 galactic Per Second-epoch detections are separated by 2.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J029.2403+56.2344 | 01:57:00.37 +56:14:14.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0V 1932MeUpp..55....1S BD+55 447
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 02 27.1856* 01 57 01.66 +56 14 15.7 11.3 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
ATO J029.2403+56.2344,2461098.6857,11.32,0.05,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 J029.2403+56.2344 20260227.1857 11.32CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:57:01.66 +56:14:15.7 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 11.18 02:00:21.48 +58:23:30.3
131.87770 -3.27786 galactic Cas Second-epoch detections are separated by 1.1" and 2.8 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 505500234660287232 | 02:00:22.47 +58:23:30.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1960IzKry..24..160B [B60] +58 617
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 02 27.1856* 02 00 21.48 +58 23 30.3 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
Gaia DR3 505500234660287232,2461098.6857,11.18,0.05,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 505500234660287232 20260227.1857 11.18CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:00:21.48 +58:23:30.3 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 9.43 02:04:05.89 +49:42:42.5
134.80269 -11.47783 galactic Per Second-epoch detections are separated by 3.0" and 3.8 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 | ATO J031.0092+49.7114 | 02:04:05.35 +49:42:39.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1856* 02 04 05.89 +49 42 42.5 9.4 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
ATO J031.0092+49.7114,2461098.6857,9.43,0.05,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
ATO J031.0092+49.7114 20260227.1857 9.43CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:04:05.89 +49:42:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 12.59 02:02:45.48 +48:39:18.7
134.89154 -12.55339 galactic Per Second-epoch detections are separated by 5.2" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 356809154057238656 | 02:02:44.86 +48:39:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (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 02 27.1856* 02 02 45.48 +48 39 18.7 12.6 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 356809154057238656,2461098.6857,12.59,0.05,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 356809154057238656 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:02:45.48 +48:39:18.7 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 01 53 22.51 +56 41 49.4 13.1 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
ZTF J015320.61+564151.0,2461098.6857,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J015320.61+564151.0 20260227.1857 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:53:22.51 +56:41:49.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.20 02:30:08.24 +57:48:49.6
135.79360 -2.57211 galactic Per Second-epoch detections are separated by 3.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.5373+57.8181 | 02:30:08.24 +57:48:49.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1856* 02 30 08.24 +57 48 49.6 13.2 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
ATO J037.5373+57.8181,2461098.6857,13.20,0.05,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 J037.5373+57.8181 20260227.1857 13.20CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:30:08.24 +57:48:49.6 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.38 02:45:18.56 +57:37:52.4
137.72542 -1.93264 galactic Cas Second-epoch detections are separated by 2.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J041.3244+57.6306 | 02:45:18.56 +57:37:52.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1856* 02 45 18.56 +57 37 52.4 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J041.3244+57.6306,2461098.6857,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J041.3244+57.6306 20260227.1857 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:45:18.56 +57:37:52.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.43 02:01:26.00 +50:25:11.4
134.18339 -10.91650 galactic Per Second-epoch detections are separated by 2.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J030.3554+50.4190 | 02:01:25.31 +50:25:08.7 (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 02 27.1856* 02 01 26.00 +50 25 11.4 13.4 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
ATO J030.3554+50.4190,2461098.6857,13.43,0.05,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
ATO J030.3554+50.4190 20260227.1857 13.43CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:01:26.00 +50:25:11.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.54 02:02:51.59 +58:02:51.1
132.28822 -3.52090 galactic Per Second-epoch detections are separated by 3.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J030.7094+58.0423 | 02:02:48.62 +58:02:35.8 (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 02 27.1856* 02 02 51.59 +58 02 51.1 13.5 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
ATO J030.7094+58.0423,2461098.6857,13.54,0.05,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
ATO J030.7094+58.0423 20260227.1857 13.54CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:02:51.59 +58:02:51.1 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 03 15 40.81 +51 11 16.4 13.9 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 442838139273214848,2461098.6857,13.87,0.05,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
Gaia DR3 442838139273214848 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:40.81 +51:11:16.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.80 02:42:52.38 +48:55:46.4
141.09456 -9.97254 galactic Per Second-epoch detections are separated by 2.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J040.7288+48.9207 | 02:42:52.38 +48:55:46.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1856* 02 42 52.38 +48 55 46.4 13.8 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
ATO J040.7288+48.9207,2461098.6857,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J040.7288+48.9207 20260227.1857 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:42:52.38 +48:55:46.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 06 19.70 +48 49 32.4 13.8 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
ASASSN-V J020619.10+484927.7,2461098.6857,13.79,0.05,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
ASASSN-V J020619.10+484927.7 20260227.1857 13.79CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:19.70 +48:49:32.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 41 07.96 +55 12 59.9 11.9 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
V0363 Per,2461098.6857,11.94,0.05,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
V0363 Per 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:41:07.96 +55:12:59.9 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 19 55.81 +53 28 08.8 12.9 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
NSVS J0219559+532808,2461098.6857,12.92,0.05,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 J0219559+532808 20260227.1857 12.92CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:19:55.81 +53:28:08.8 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 32 11.60 +49 54 43.5 12.0 U And 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 J0232117+495440,2461098.6857,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0232117+495440 20260227.1857 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:32:11.60 +49:54:43.5 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 50 00.08 +53 38 56.3 12.8 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
NSVS J0250001+533854,2461098.6857,12.79,0.05,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
NSVS J0250001+533854 20260227.1857 12.79CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:50:00.08 +53:38:56.3 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 22 56.64 +51 34 15.5 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
V0759 Per,2461098.6857,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0759 Per 20260227.1857 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:22:56.64 +51:34:15.5 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 43 37.56 +53 05 01.6 12.9 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
NSVS J0243375+530503,2461098.6857,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0243375+530503 20260227.1857 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:43:37.56 +53:05:01.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 03 12 59.67 +55 44 11.9 12.7 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
NSVS 1951420,2461098.6857,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1951420 20260227.1857 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:12:59.67 +55:44:11.9 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 47 19.78 +55 04 00.2 12.9 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
NSVS J0247199+550360,2461098.6857,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0247199+550360 20260227.1857 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:47:19.78 +55:04:00.2 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 42 06.27 +55 53 27.7 13.1 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
2MASS J02420618+5553297,2461098.6857,13.10,0.05,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
2MASS J02420618+5553297 20260227.1857 13.10CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:42:06.27 +55:53:27.7 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 13.06 02:47:28.32 +53:09:14.3
139.92894 -5.84524 galactic Per Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:47:28.32 +53:09:14.3 (user input) | T | P | (position from user input) SpType: F4 (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 02 27.1856* 02 47 28.32 +53 09 14.3 13.1 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
target,2461098.6857,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.1857 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:47:28.32 +53:09:14.3 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 18 31.15 +56 04 11.5 12.0 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
DF Per,2461098.6857,12.02,0.05,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
DF Per 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:18:31.15 +56:04:11.5 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 50 25.41 +54 45 23.3 12.3 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
NSVS 1931148,2461098.6857,12.26,0.05,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
NSVS 1931148 20260227.1857 12.26CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:50:25.41 +54:45:23.3 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 32 46.55 +56 29 27.8 13.3 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,2461098.6857,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LR Per 20260227.1857 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:32:46.55 +56:29:27.8 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 21 34.90 +53 10 06.9 12.1 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
ASASSN-V J022134.44+531006.6,2461098.6857,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022134.44+531006.6 20260227.1857 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:21:34.90 +53:10:06.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 9.95 03:41:25.10 +56:55:32.8
144.57097 1.37424 galactic Cam Second-epoch detections are separated by 0.4" and 3.1 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 448786359739139328 | 03:41:25.01 +56:55:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1928AnHar.100...49C HD 237166 J-Ks=0.309+/-0.037 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 448786359739139328,2461098.6857,9.95,0.05,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
Gaia DR3 448786359739139328 20260227.1857 9.95CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:25.10 +56:55:32.8 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 56 42.34 +50 33 28.4 13.6 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
NSVS J0256419+503326,2461098.6857,13.60,0.05,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
NSVS J0256419+503326 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:42.34 +50:33:28.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 38 23.71 +55 07 25.8 11.7 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
ASASSN-V J023823.53+550725.0,2461098.6857,11.74,0.05,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
ASASSN-V J023823.53+550725.0 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:38:23.71 +55:07:25.8 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 18 51.55 +55 21 05.4 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
NSVS J0218515+552110,2461098.6857,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0218515+552110 20260227.1857 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:18:51.55 +55:21:05.4 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1857 2461098.6857 11.66 03:46:19.19 +57:47:36.6
144.56738 2.46496 galactic Cam Second-epoch detections are separated by 0.7" and 3.1 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 448931563997893120 | 03:46:19.21 +57:47:36.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1956ApJS....2..298M LF 6 +57 49 J-Ks=0.190+/-0.026 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 448931563997893120,2461098.6857,11.66,0.05,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 448931563997893120 20260227.1857 11.66CV 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:19.19 +57:47:36.6 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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 02 27.1856* 02 57 02.96 +52 43 56.5 12.8 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
NSVS J0257030+524404,2461098.6857,12.85,0.05,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
NSVS J0257030+524404 20260227.1857 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:02.96 +52:43:56.5 ;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_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20_00sec_-14_90C_LIGHT_0012_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: 2461032.75818454 23.12.2025 06:11:37.144 /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
First image: 2461032.75818454 23.12.2025 06:11:37.144 /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
Last image: 2461098.68593697 27.02.2026 04:27:34.954 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 36
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 26948
Objects passed selection criteria: 26848
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 21168.5
Average stars matched: 20619.2 (97.4053 %)
Memory usage VmPeak: 130700 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Feb 27 01:54:33 CST 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: 2461032.75818454 23.12.2025 06:11:37.144 /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
First image: 2461032.75818454 23.12.2025 06:11:37.144 /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
Last image: 2461098.68593697 27.02.2026 04:27:34.954 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 863
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.37
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 67 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): 171998
Objects passed selection criteria: 171617
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 136958
Average stars matched: 132448 (96.7072 %)
Memory usage VmPeak: 1994928 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Feb 27 01:58:39 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE=
FRAME_EDGE_OFFSET_PIX= 100
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Per-01-Q2b1x1
#######################################
########### Starting Per-01-Q2b1x1 ###########
Processing Per-01-Q2b1x1
server tau has sufficient free disk space available: 752545 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 752545 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.png' -> 'transient_report/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits_preview.png'
Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
renamed 'Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.png' -> 'transient_report/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits_preview.png'
Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 584.4322
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 848.7675
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 2614.8274
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 905.2261
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 2619.7623
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 906.0663
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 4.47413
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
SExtractor catalog cache: saved Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat to cache
SExtractor catalog cache: saved Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.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: 2461098.68536862
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_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits exists and is non-empty
Saving wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits to local_wcs_cache/
'wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits' -> 'local_wcs_cache/wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits'
wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits exists and is non-empty
Saving wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits to local_wcs_cache/
'wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits' -> 'local_wcs_cache/wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits'
wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits exists and is non-empty
Saving wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits to local_wcs_cache/
'wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits' -> 'local_wcs_cache/wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits'
wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits exists and is non-empty
Saving wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits to local_wcs_cache/
'wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits' -> 'local_wcs_cache/wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.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 02:49:25.719 +53:59:48.71
Second-epoch image center 02:49:23.224 +54:01:07.23
Angular distance between the image centers 0.02 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 02:49:25.719 +53:59:48.71
Second-epoch image center 02:49:21.000 +54:01:07.45
Angular distance between the image centers 0.02 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 02:49:23.224 +54:01:07.23
Second-epoch second image center 02:49:21.000 +54:01:07.45
Angular distance between the image centers 0.00545 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits &> /tmp/tmp.E3VfteTBIJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits &> /tmp/tmp.M7jZJZXSPA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits &> /tmp/tmp.jY9yGXySD5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits &> /tmp/tmp.WG8Upux9wH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.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_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits and wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.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_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits and wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat
Found non-empty wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits and wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat
The reference image (wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits) and catalog (wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat) found
'wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.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 12704 out of 28578 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.965449
a=0.000000 b=1.000000 c=22.965449
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
2.2 pix Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
2.7 pix Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
2.6 pix Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
Limiting magnitude estimates:
15.3 mag. Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
15.3 mag. Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
14.4 mag. Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
14.4 mag. Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.E3VfteTBIJ (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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits' -> 'wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
WCS_IMAGE_NAME=wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
WCS-calibrated image found: wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
Checking if the catalog wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits alredy exist and is non-empty...
Catalog wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
WCS catalog name: wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3275, passed=28578
Got 28578 stars (including 25264 good ones) from the SExtractor catalog wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat
util/solve_plate_with_UCAC5 got 28578 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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 969 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: 0.40"
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_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits -region wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.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.M7jZJZXSPA (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/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits' -> 'wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
Checking if the catalog wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
WCS catalog name: wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3210, passed=28692
Got 28692 stars (including 25451 good ones) from the SExtractor catalog wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat
util/solve_plate_with_UCAC5 got 28692 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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 964 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits -region wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.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.jY9yGXySD5 (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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
WCS-calibrated image found: wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
Checking if the catalog wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
WCS catalog name: wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1232, passed=13995
Got 13995 stars (including 12755 good ones) from the SExtractor catalog wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 13995 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits -region wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.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.WG8Upux9wH (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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
Checking if the catalog wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
WCS catalog name: wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1231, passed=13918
Got 13918 stars (including 12679 good ones) from the SExtractor catalog wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 13918 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits -region wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Per-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out32076.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out21551.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 31877_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31877_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:54:12.23 +57:32:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 2.373 506093970934669952 028.54973537436 +57.53608636485 10.6484 10.0344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31878_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31878_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:01:45.54 +58:32:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 5.529 505506316333841536 030.44247038906 +58.54119712419 10.1140 9.4115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31879_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31879_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 31880_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31880_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:00:22.01 +58:23:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 3.856 505500234660287232 030.09363997943 +58.39182172122 9.6831 9.0500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31881_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31881_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:52:56.40 +57:36:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 5.028 505734568071990144 028.23748035692 +57.61170805650 9.4205 8.7330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31891_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31891_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:42.52 +57:17:22.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31901_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31901_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:45:46.95 +57:52:18.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31902_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31902_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:43:00.38 +57:33:56.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31921_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31921_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:45:51.15 +57:34:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.26, MAG_FAINT_SEARCH_LIMIT=11.24)GAIADR2_OUTPUT=# 2.695 448920049182880640 056.46177208809 +57.57023267101 9.2798 9.0358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31924_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31924_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:17.85 +57:31:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.36, MAG_FAINT_SEARCH_LIMIT=11.34)GAIADR2_OUTPUT=# 1.292 448872911923119616 056.57372419199 +57.52000208430 9.3758 9.1561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31936_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31936_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:06.49 +56:59:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 0.399 448823090302109056 056.52689299701 +56.99072982122 9.7210 9.2806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31944_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31944_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:53.50 +57:44:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 2.490 448928712139619712 056.72169720386 +57.73390516272 9.7390 9.4198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31950_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31950_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:43:04.94 +57:59:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 0.737 449134836208034688 055.77032741414 +57.99926327767 9.7873 9.2261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31979_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31979_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:08.19 +57:03:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 0.797 448824705209481088 056.53377919816 +57.06255002849 10.2375 9.8679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31983_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31983_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:44:03.51 +49:12:59.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31990_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31990_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:23:18.89 +57:12:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 1.362 458413511759296896 035.82811496311 +57.21622752754 10.9786 10.6151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31992_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 31992_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:41:57.02 +58:08:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 1.288 449128204777727872 055.48695039904 +58.13359428616 10.4528 10.0727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32021_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 32021_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:19:09.92 +57:06:27.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)
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Considering the candidate 32057_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 32057_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:19.49 +57:47:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 2.440 448931563997893120 056.58003068378 +57.79338342774 10.7485 10.3665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32059_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 32059_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:45:33.61 +57:08:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 0.154 448828965817016704 056.39012047010 +57.13833593519 10.7604 10.1251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32076_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 32076_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:31:22.93 +56:52:56.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)
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Considering the candidate 32103_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 32103_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:37.64 +57:52:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.973 448934072258736640 056.65888219974 +57.87334218021 10.4876 9.3770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32108_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 32108_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:45.03 +57:56:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.944 448934931252157312 056.68732960591 +57.94978976404 10.9585 10.3934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32127_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 32127_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:44:26.96 +57:58:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.233 449131675112063872 056.11296893437 +57.97985571103 10.8980 10.0257 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 32135_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 32135_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:44:31.06 +57:27:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.058 448895177027608448 056.12896562807 +57.45297323685 11.2067 10.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21551_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 21551_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Per-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:19:14.40 +51:15:28.2
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
SExtractor catalog cache: saved Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat to cache
SExtractor catalog cache: saved Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
Creating symlink local_wcs_cache/wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
Creating symlink local_wcs_cache/wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
Creating symlink local_wcs_cache/wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
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_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits exists and is non-empty
wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits exists and is non-empty
wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits exists and is non-empty
wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.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 02:49:25.719 +53:59:48.71
Second-epoch image center 02:49:23.224 +54:01:07.23
Angular distance between the image centers 0.02 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 02:49:25.719 +53:59:48.71
Second-epoch image center 02:49:21.000 +54:01:07.45
Angular distance between the image centers 0.02 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 02:49:23.224 +54:01:07.23
Second-epoch second image center 02:49:21.000 +54:01:07.45
Angular distance between the image centers 0.00545 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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits &> /tmp/tmp.nmXbp2FqTw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits &> /tmp/tmp.3x8TSH6l3k
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits &> /tmp/tmp.ZScwjH2HUD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits &> /tmp/tmp.Tsg3FlwJiL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.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_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits and wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.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_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits and wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat
Found non-empty wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits and wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat
The reference image (wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits) and catalog (wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat) found
'wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.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 12888 out of 187490 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.831256
a=0.000000 b=1.000000 c=22.831256
From vast_summary.log: estimated ref. image limiting mag.: -7.37
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 703 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
2.1 pix Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
2.5 pix Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
2.4 pix Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
Limiting magnitude estimates:
15.5 mag. Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
15.4 mag. Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
14.5 mag. Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
14.5 mag. Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 13.8 (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.nmXbp2FqTw (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/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits' -> 'wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
WCS_IMAGE_NAME=wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
WCS-calibrated image found: wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
Checking if the catalog wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits alredy exist and is non-empty...
Catalog wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits
WCS catalog name: wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=26738, passed=187432
Got 187432 stars (including 160397 good ones) from the SExtractor catalog wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat
util/solve_plate_with_UCAC5 got 187432 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 970 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: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.36"
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_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits -region wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-01-Q2b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.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.3x8TSH6l3k (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/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits' -> 'wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
Checking if the catalog wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits
WCS catalog name: wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=40, blended=26065, passed=184075
Got 184075 stars (including 157736 good ones) from the SExtractor catalog wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat
util/solve_plate_with_UCAC5 got 184075 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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 964 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits -region wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-01-Q2b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.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.ZScwjH2HUD (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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
WCS-calibrated image found: wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
Checking if the catalog wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits
WCS catalog name: wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=8382, passed=89265
Got 89265 stars (including 80789 good ones) from the SExtractor catalog wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 89265 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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: 0.54"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits -region wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-01-Q2b1x1_2026-02-26_22-26-45_20.00sec_-14.90C_LIGHT_0012.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.Tsg3FlwJiL (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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.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_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
Checking if the catalog wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat corresponding to the image wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits
WCS catalog name: wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=8657, passed=90731
Got 90731 stars (including 81974 good ones) from the SExtractor catalog wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 90731 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q2b1x1_224144_TTUQ2b1x1_7926_PyM2Ytvm/Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits -region wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Per-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out10331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out164749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178097.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211689.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213173.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213174.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213185.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out76844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out211588.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out212036.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out212802.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out03176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out182631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97368.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 104s
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: 43s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211487_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211487_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:37:35.55 +52:31:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.489 443958094944107264 054.39776127445 +52.52842818441 13.7354 13.0379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211490_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211490_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:24:51.70 +54:43:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.578 446689006949528576 051.21532234600 +54.72432114357 13.6415 12.5287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211493_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211493_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211495_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211495_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:42:14.35 +55:24:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.356 445583001331038208 055.55974534605 +55.40776307719 14.0493 13.3627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211496_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211496_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:44:10.10 +57:00:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 3.092 448832504870220160 056.04363885435 +57.01641220116 13.6165 12.9178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211499_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211499_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:57:14.84 +55:01:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.317 504481120512424832 029.31194204018 +55.02933271956 12.7220 12.0016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211505_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211505_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:57:58.14 +56:42:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.553 504887768016637312 029.49119219163 +56.71575953218 12.8972 12.6396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211506_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211506_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:05:51.40 +52:53:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.185 359971830535922432 031.46399643450 +52.88596494005 13.1095 12.5979 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 211518_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211518_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:05:50.37 +49:13:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.374 358140486541653888 031.45978552145 +49.23075256940 12.5920 12.0266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211520_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211520_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 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 211524_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211524_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:57:54.16 +54:08:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 4.440 408320277389007616 029.47378171799 +54.13453421338 12.7452 12.2422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211526_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211526_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:55:15.49 +55:14:32.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
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Considering the candidate 211533_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211533_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:52:01.33 +49:47:16.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
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Considering the candidate 211534_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211534_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:58:28.93 +57:13:28.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)
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Considering the candidate 211536_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211536_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:03:50.96 +51:21:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.818 359354351677332480 030.96188991210 +51.36108886386 12.9898 12.2184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211544_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211544_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:00:39.31 +51:29:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.147 359415305852941824 030.16194189557 +51.49233012961 12.4485 11.9018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211545_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211545_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 211548_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211548_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:58:26.59 +49:14:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.092 439206108767147136 044.61022279371 +49.24330821091 14.0838 13.1135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211549_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211549_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:06:14.40 +49:16:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.393 358161308543102976 031.55960736141 +49.26956758363 12.5496 11.9112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211552_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211552_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:08:11.64 +57:53:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.593 506726258843086976 032.04802307830 +57.89074846174 12.8881 12.4143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211554_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211554_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211555_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211555_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:01:11.62 +51:10:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 5.838 359337511106934016 030.29582996086 +51.17803876510 12.7130 12.1935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211559_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211559_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:57:57.82 +56:03:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.727 504828261253300864 029.49163913330 +56.05331512937 12.3378 11.8985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211560_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211560_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:20:15.58 +48:53:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.824 435640255120547840 050.06459935409 +48.88801065550 13.2677 12.6510 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 211562_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211562_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:03:24.42 +57:37:32.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 211569_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211569_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:13:00.20 +57:00:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.528 460084735066650112 048.25024130164 +57.00598735838 13.7772 13.0438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211572_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211572_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:59:21.03 +58:03:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.218 505466523450645504 029.83976931935 +58.05109653514 12.3475 11.8219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211575_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211575_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 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 211577_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211577_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:03.34 +49:27:51.3 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 211579_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211579_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:54:48.13 +56:32:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.560 504906017342671232 028.70117735339 +56.54464680590 12.0116 11.1209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211585_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211585_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:58:54.25 +58:17:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.173 505486623896175232 029.72596016879 +58.28428803566 12.2173 11.6511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211586_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211586_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211588_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211588_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:56:54.04 +55:32:27.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 211590_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211590_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211592_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211592_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:06:34.66 +58:27:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 0.613 506946023727737472 031.64433782323 +58.45783491831 12.4885 11.9864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211597_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211597_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:02:00.57 +57:44:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.314 505396949284173312 030.50142961733 +57.73621298543 12.4849 11.8486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211599_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211599_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:58:58.59 +56:23:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.690 504862861510741632 029.74215917126 +56.39122820335 12.5128 12.0181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211602_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211602_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:12:23.36 +56:27:57.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)
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Considering the candidate 211603_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211603_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:00:39.32 +51:04:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.870 359335071565513984 030.16139685591 +51.07488290785 12.5970 12.3620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211604_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211604_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211607_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211607_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211609_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211609_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211612_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211612_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:10:04.62 +51:07:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.830 358922617269153664 032.52040272773 +51.12088696556 13.1465 12.5622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211614_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211614_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:58:24.02 +54:34:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.868 408345050760704896 029.60289181050 +54.58155760158 12.0128 11.2207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211615_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211615_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211616_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211616_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:00:27.91 +56:11:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.080 504657630793869952 030.11563275161 +56.18281044023 12.4846 11.9386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211617_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211617_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:32:31.78 +56:40:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.676 457772530837500928 038.13145649975 +56.67475742296 13.6208 12.9367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.676#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211618_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211618_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:59:53.19 +58:24:33.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)
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Considering the candidate 211620_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211620_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 211623_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211623_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211628_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211628_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 211631_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211631_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:45:32.61 +57:14:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.451 448841507121469440 056.38522083418 +57.24405732985 12.9464 12.3945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211633_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211633_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:59:55.29 +54:25:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.078 504404055921113472 029.97946018497 +54.42697068966 12.3706 11.6926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211634_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211634_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211636_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211636_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211637_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211637_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:25:27.19 +49:18:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.409 441481067046296832 051.36323476052 +49.30958266029 12.8477 11.8763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211639_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211639_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:07:31.55 +58:36:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.308 506784567319298816 031.88253907183 +58.59994419415 12.4134 11.5664 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 211640_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211640_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 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 211641_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211641_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:59:48.73 +55:25:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.708 504472912835752448 029.95139253235 +55.42130231983 12.6191 12.0794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211642_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211642_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211644_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211644_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211645_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211645_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211647_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211647_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:16:33.53 +55:06:48.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 211651_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211651_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:25:20.76 +54:01:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.585 455592542877500672 036.33814683212 +54.01940242427 13.9587 13.4185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211656_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211656_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:43:19.14 +57:18:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 0.861 448889542037387648 055.82983656883 +57.30784886926 13.0006 12.4408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211660_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211660_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:01:24.45 +52:18:04.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 211662_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211662_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:00:16.36 +57:49:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.724 505412308087142400 030.06704526688 +57.82386858097 12.2757 11.9330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211664_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211664_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:29:05.64 +55:11:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.387 457222053471332608 037.27242197882 +55.18578080848 13.6941 13.0963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211670_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211670_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211674_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211674_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:19:34.26 +52:31:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.234 455030000937938688 034.89229199013 +52.53194957362 13.4833 13.2153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211679_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211679_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211680_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211680_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211685_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211685_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:12:34.48 +49:03:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.776 355178509594080512 033.14164727165 +49.05926562334 12.7611 12.0172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211687_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211687_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:15:20.96 +49:42:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.604 436511858603297280 048.83707416653 +49.71628660781 13.2305 12.2506 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 211688_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211688_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211689_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211689_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:58:36.67 +53:50:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.989 360251965483270272 029.65045285655 +53.84151109206 12.2680 11.5829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211690_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211690_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:04:38.35 +58:23:05.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)
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Considering the candidate 211692_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211692_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211695_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211695_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:54:01.70 +56:47:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.287 504925464954327424 028.50827574508 +56.80024948127 11.8469 10.9934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211696_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211696_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:06:34.82 +50:23:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.264 358512430709503232 031.64505023176 +50.38762135960 12.2919 11.5265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211697_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211697_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211698_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211698_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211700_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211700_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 211701_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211701_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:58:00.99 +55:09:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 4.918 504486519292501248 029.50201110515 +55.15436161773 12.0912 11.4851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211702_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211702_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 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 211708_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211708_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:05:04.17 +58:39:35.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 211709_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211709_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:56:07.71 +56:56:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 5.699 504941300489000704 029.03502391190 +56.94284105690 11.8363 11.0421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211711_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211711_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211717_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211717_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:57:06.60 +56:58:47.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)
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Considering the candidate 211721_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211721_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 211722_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211722_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:25:25.68 +53:45:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.153 455491177345486464 036.35697177680 +53.75976342315 13.2518 12.8357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211726_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211726_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211730_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211730_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:02:32.18 +58:04:02.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 211731_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211731_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:38:40.99 +50:45:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.174 451046508968078976 039.67078144161 +50.75503533267 13.2079 12.6527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211732_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211732_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211733_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211733_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:59:46.58 +54:01:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.479 360277593548654208 029.94294215481 +54.02520317069 11.9576 11.5208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211734_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211734_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:58:53.58 +55:20:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 5.316 504512770132365952 029.72069129662 +55.34211011077 11.8989 11.2660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211735_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211735_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211737_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211737_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211739_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211739_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:27:47.46 +51:51:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.862 451764490061422592 036.94754314778 +51.85380674662 13.4142 12.8895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211740_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211740_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211744_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211744_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 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 211748_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211748_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211750_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211750_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211753_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211753_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211754_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211754_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211756_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211756_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211762_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211762_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:00:01.59 +56:02:12.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 211763_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211763_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211767_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211767_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 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 211768_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211768_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211769_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211769_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211770_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211770_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:59:52.10 +52:22:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 5.294 360020105969407616 029.96491968045 +52.38129747474 11.7349 11.2468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211772_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211772_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211773_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211773_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 211781_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211781_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211784_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211784_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:01:24.59 +51:48:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.981 359800886539176576 030.35352912789 +51.80330886507 11.5618 10.7831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211785_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211785_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:41:03.93 +52:21:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.160 452912448924705664 040.26688731928 +52.35889471684 13.0118 12.5214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211786_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211786_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211789_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211789_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:46:41.17 +52:11:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 4.004 452673270785584512 041.66973999020 +52.19657751545 13.1233 12.5422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211791_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211791_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:58:49.76 +55:28:38.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 211792_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211792_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 01:52:46.88 +58:10:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 4.682 506174372724251520 028.19300254146 +58.17939767961 11.2118 10.4145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211793_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211793_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211796_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211796_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211797_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211797_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211798_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211798_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211800_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211800_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:39:43.88 +56:14:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.319 448685475247423872 054.93271118340 +56.24305425924 11.6967 11.1641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211803_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211803_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211807_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211807_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211809_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211809_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211823_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211823_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:45:46.83 +57:52:18.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 211830_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 211830_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 211845_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211845_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:45:50.95 +57:34:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.15, MAG_FAINT_SEARCH_LIMIT=11.13)GAIADR2_OUTPUT=# 1.037 448920049182880640 056.46177208809 +57.57023267101 9.2798 9.0358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211848_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211848_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:17.72 +57:31:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.26, MAG_FAINT_SEARCH_LIMIT=11.24)GAIADR2_OUTPUT=# 0.286 448872911923119616 056.57372419199 +57.52000208430 9.3758 9.1561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211849_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211849_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:13:01.25 +58:56:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.22, MAG_FAINT_SEARCH_LIMIT=11.20)GAIADR2_OUTPUT=# 0.515 461959191936195200 048.25493367184 +58.94040901095 9.9019 9.3535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211869_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211869_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:53.20 +57:44:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.70, MAG_FAINT_SEARCH_LIMIT=11.68)GAIADR2_OUTPUT=# 0.346 448928712139619712 056.72169720386 +57.73390516272 9.7390 9.4198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211871_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211871_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:56:57.14 +54:37:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 1.333 453431109172256000 044.23747719879 +54.62627065720 11.1848 10.6832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211881_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211881_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 211883_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211883_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 211885_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211885_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 211886_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211886_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 211892_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211892_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 211909_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211909_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 211913_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211913_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 211917_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211917_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:03:54.59 +49:02:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 2.176 358319122821726336 030.97660676276 +49.04046243240 9.7252 9.0421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211919_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211919_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:05:21.60 +48:40:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 4.773 356610997149971200 031.34137322454 +48.67696724080 10.1206 9.9536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211921_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211921_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 211924_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211924_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 211928_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211928_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 211929_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211929_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 211940_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211940_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 211941_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211941_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 211942_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211942_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 211945_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211945_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 211954_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211954_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 211955_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211955_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 211956_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211956_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 211961_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211961_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:02:16.48 +49:51:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 0.820 358405473141836160 030.56846738080 +49.86558955281 9.9090 8.8040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211962_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211962_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 211971_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211971_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 211979_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211979_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 211980_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211980_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 211981_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 211981_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 212003_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212003_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 212007_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212007_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 212022_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212022_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 212025_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212025_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 212036_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212036_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:31:23.19 +56:52:57.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)
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Considering the candidate 212041_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212041_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 212046_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212046_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:44.88 +57:56:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.841 448934931252157312 056.68732960591 +57.94978976404 10.9585 10.3934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212050_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212050_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 212051_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212051_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:07:13.86 +49:02:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 0.504 436206400530778112 046.80754033575 +49.04747339030 11.6166 10.7825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212058_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212058_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 212063_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212063_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 212067_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212067_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 212069_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212069_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 212074_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212074_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 212085_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212085_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 212091_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212091_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 212092_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212092_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 212096_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212096_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:27:59.04 +49:01:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.257 441415165068758400 051.99546789089 +49.01951984588 11.4735 11.0492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212098_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212098_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 212107_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212107_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 212109_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212109_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 212111_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212111_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 212112_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212112_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 212114_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212114_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 212115_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212115_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:45:58.46 +57:50:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.546 448932629149769984 056.49359766927 +57.83626512750 11.2394 10.7226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212121_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212121_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:25:52.47 +50:15:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.449 451517095648994432 036.46811849473 +50.26595722160 11.6557 10.8465 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 212128_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212128_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 212145_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212145_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 212153_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212153_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 212156_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212156_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 212162_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212162_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 212170_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212170_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 212174_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212174_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 212184_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212184_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:19:02.38 +50:04:24.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212195_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212195_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:12.76 +57:43:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.702 448930773715579904 056.55343791471 +57.73148059879 11.4682 10.9961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212203_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212203_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 212205_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212205_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 212208_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212208_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 212213_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212213_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 212217_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212217_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 212225_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212225_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 212228_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212228_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:45:31.14 +57:59:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.090 448949156175241856 056.37979337108 +57.98451813039 11.5750 10.9866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212237_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212237_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 212245_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212245_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 212246_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212246_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 212249_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212249_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 212269_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212269_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:29:55.87 +55:20:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.068 457224183775001472 037.48236481842 +55.33796847324 12.4836 12.0468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212272_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212272_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 212274_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212274_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 212277_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212277_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 212289_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212289_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 212293_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212293_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:28.53 +57:29:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.576 448871915490724864 056.61889076477 +57.48361813850 11.6511 11.2161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212304_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212304_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 212310_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212310_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 212311_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212311_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 212324_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212324_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:31:15.21 +58:01:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 1.328 458095890338480384 037.81275841924 +58.01777319227 12.3607 11.8157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212325_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212325_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:21:50.80 +57:15:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.197 458456427074516992 035.46115348709 +57.26448861116 12.5698 11.8758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212328_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212328_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:24:10.23 +49:48:11.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 212334_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212334_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 212360_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212360_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:50:59.28 +55:55:26.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 212365_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212365_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:02:49.79 +49:34:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.878 358397428665418880 030.70725024766 +49.57227389358 11.5841 10.7773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212368_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212368_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 212374_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212374_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 212392_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212392_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 212400_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212400_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 212402_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212402_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 212416_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212416_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 212418_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212418_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 212419_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212419_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 212424_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212424_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 212426_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212426_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 212429_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212429_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 212430_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212430_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 212436_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212436_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:48:56.79 +58:00:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.679 460991969602052096 042.23602855814 +58.00562919696 12.7639 12.2173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212446_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212446_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 212448_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212448_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 212470_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212470_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 212471_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212471_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:22:06.03 +55:17:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.173 455957305861974272 035.52604334146 +55.29421822963 12.6405 11.8550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212478_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212478_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:37.76 +57:27:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 0.666 448868887532455680 056.65730061247 +57.45356595656 12.0612 11.6677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212483_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 212483_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 212487_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212487_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 212492_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212492_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 212495_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212495_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 212500_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212500_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:50:54.18 +55:55:49.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 212503_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212503_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 212514_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212514_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:33:28.87 +57:34:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.699 458024765678604800 038.36876029210 +57.57654912739 12.7423 12.2296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212515_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212515_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:18:46.51 +50:11:56.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212517_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212517_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 212518_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212518_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:02:15.76 +49:44:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.162 358402277686236160 030.56466370502 +49.73446288809 11.4108 10.2463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212524_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212524_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:32:02.56 +48:57:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 0.182 450456994638237824 038.01071113919 +48.96484778437 12.5550 11.9849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212532_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212532_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 212533_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212533_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:27:47.48 +50:35:37.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212534_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212534_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:44:10.84 +58:01:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.476 449132740263937024 056.04467704377 +58.02657135131 12.0858 11.6553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212536_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212536_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 212537_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212537_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:56:30.31 +57:55:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.016 460768184624537088 044.12668891273 +57.93056463570 12.9864 12.3207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212544_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212544_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 212552_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212552_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:24:14.43 +49:49:03.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 212555_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212555_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 212560_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212560_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 212561_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212561_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 212566_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212566_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 212578_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212578_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:25:42.50 +53:56:43.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212591_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212591_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 212592_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212592_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:33:32.57 +56:18:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.080 457374645069998976 038.38658932678 +56.30624734405 13.0011 12.4121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212599_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212599_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 212601_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212601_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 212602_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212602_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 212608_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212608_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:22:16.40 +56:34:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 2.083 458284108680702208 035.56860121486 +56.58235714465 12.9184 12.5950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212628_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212628_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 212633_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212633_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:24:13.53 +49:48:08.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 212642_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212642_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 212643_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212643_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:25:13.21 +52:21:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.669 452024387123354752 036.30435622972 +52.36333834760 13.0596 12.5857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212647_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212647_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:23:40.23 +52:42:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.918 452048060982938624 035.91806659751 +52.70057166111 13.0092 12.2712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212649_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212649_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:48:50.99 +58:01:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.120 461003789352033920 042.21187174035 +58.03068424512 12.8084 12.0731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212650_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212650_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 212651_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212651_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 212652_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212652_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 212653_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212653_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 212669_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212669_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:09:35.98 +57:56:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.075 506686195386369536 032.40075583609 +57.94873698077 12.5431 12.1438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212670_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212670_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 212675_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212675_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 212676_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212676_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 212677_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212677_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 212678_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212678_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:06:59.06 +49:04:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.632 358146602575090560 031.74583927460 +49.08301732230 11.7692 11.0536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212679_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212679_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 212687_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212687_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 212697_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212697_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 212698_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212698_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 212704_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212704_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 212708_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212708_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:05.62 +57:39:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.665 448881192619939200 056.77321253003 +57.65421224959 12.2908 11.8693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212709_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212709_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 212712_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212712_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 212714_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212714_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 212720_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212720_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:25.75 +57:44:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.157 448882051613356160 056.85779712103 +57.74160291637 12.1943 11.6420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212721_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212721_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:32:46.43 +50:17:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.081 450813721740939392 038.19435747272 +50.28820198777 13.1034 12.3286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212726_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212726_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 212729_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212729_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 212734_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212734_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:15:30.99 +50:54:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.843 442830648850617472 048.87871964098 +50.90666760041 13.0423 12.3701 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 212740_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212740_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:28:12.44 +49:03:37.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212741_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212741_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 212743_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212743_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:44:03.94 +49:15:14.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212750_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212750_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 212752_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212752_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 212759_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212759_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 212762_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212762_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 212763_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212763_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 212773_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 212773_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 212779_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212779_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 212782_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212782_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:34:33.81 +50:03:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.472 450793724373586688 038.64081798729 +50.05134265836 13.1590 12.5135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212799_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212799_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 212802_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212802_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:28:48.01 +49:40:33.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 212803_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212803_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 212805_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212805_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 212811_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212811_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 212815_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212815_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 212817_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212817_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 212821_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212821_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:04:03.53 +52:32:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.718 440959176980255232 046.01502115933 +52.53367086004 12.8151 11.7589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212824_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212824_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 212825_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212825_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:30:04.56 +51:33:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.470 451696350403558912 037.51964498078 +51.56408212333 13.4462 12.8163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212828_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212828_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:29:24.32 +53:52:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.342 452595888353062400 037.35061418701 +53.87602139230 13.4987 13.0204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212833_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212833_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:03:32.53 +49:08:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.180 358323589587676928 030.88427909981 +49.13915941378 11.7004 10.8015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212834_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212834_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 212836_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212836_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 212840_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212840_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:13:04.05 +54:13:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.745 456173119374296960 033.26816933976 +54.21795316873 13.1517 12.4601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212842_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212842_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:52:03.55 +53:00:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.725 453180622381608192 043.01473949383 +53.00999560016 12.9108 11.9026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212849_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212849_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 212855_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212855_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 212856_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212856_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:04:29.11 +50:03:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.203 439358631648067584 046.12163804292 +50.05130477606 13.3724 12.7808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212857_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212857_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:32.05 +57:51:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.149 472949570872266112 056.88406754316 +57.86290186236 12.3633 11.8802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212864_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212864_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:50:57.61 +57:50:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.381 460940017677691904 042.73925522257 +57.83504812394 13.3277 12.7571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212867_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212867_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 212871_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212871_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:16:59.92 +57:02:25.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212872_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212872_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:23:19.84 +49:13:46.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212873_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212873_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 212893_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212893_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:02:31.64 +49:38:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.208 358398734335472768 030.63012666468 +49.64237182330 11.7097 10.6258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212895_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212895_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 212899_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212899_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:02:33.07 +50:14:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.473 358451549550813312 030.63721572486 +50.24509933765 11.9132 11.3452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212901_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212901_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 212909_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212909_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:28:14.11 +54:24:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.315 455629445237033216 037.05772298221 +54.41397506415 13.2123 12.6890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212912_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212912_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:44:18.66 +56:40:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.981 454781549972022272 041.07863512514 +56.66803528769 13.1363 12.1500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212914_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212914_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:37:54.69 +52:48:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.838 452237005186507904 039.47818680307 +52.80399777514 13.2867 12.4510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212917_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212917_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:15:04.94 +55:03:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.779 456607048513619200 033.77006032427 +55.06251063473 12.9650 12.4402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212919_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212919_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 212921_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212921_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 212922_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212922_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 212927_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212927_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 212929_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 212929_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 212930_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212930_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 212936_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212936_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 212943_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212943_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 212945_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212945_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:31:50.38 +57:32:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.919 458067784072721024 037.96063356876 +57.55068588161 13.4966 12.9089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212949_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212949_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:46:56.08 +56:39:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 0.779 454773475433943040 041.73345609662 +56.65684963537 13.5926 13.0665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212959_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212959_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:42:57.04 +53:29:45.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212962_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212962_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:28:12.79 +51:43:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.465 451759748417546880 037.05455046863 +51.72596327770 13.1154 12.1401 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 212964_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212964_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:11.18 +57:54:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.668 448946063807429376 056.54586736899 +57.90054132406 12.5732 12.0683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212966_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212966_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 212969_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212969_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:56:51.97 +57:34:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.465 460695341979417856 044.21650662632 +57.57990650539 13.4687 12.8282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212972_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212972_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 212977_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212977_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 212978_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212978_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:42.44 +57:34:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.798 448879062316221312 056.67724413477 +57.57866877179 12.5126 11.8532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212979_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212979_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:14.40 +57:45:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.150 448929021377233792 056.81055500952 +57.75682479951 12.4831 11.8517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212983_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212983_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:54:53.25 +50:59:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.111 440439657737466368 043.72084875318 +50.99610196218 13.5157 12.8736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212984_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212984_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:15:54.67 +50:58:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.589 442832710434809600 048.97754280092 +50.97493637352 13.3408 12.6472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212985_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212985_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 212987_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212987_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:37:02.79 +55:56:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.962 454676340453173248 039.26219950656 +55.93532883499 13.6980 13.2623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212990_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212990_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 212991_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212991_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 212992_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212992_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:37:15.17 +52:12:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.175 451445215076188800 039.31318218103 +52.20325719133 13.4081 12.5493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212993_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212993_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:32:48.38 +54:33:12.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 212994_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212994_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:44:38.18 +49:20:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.271 438832407954126848 041.15900629785 +49.34844511044 13.5545 12.9321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212999_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 212999_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 213001_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213001_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:19:16.03 +50:06:46.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 213002_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213002_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:52:38.54 +53:44:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.927 453282365865241856 043.15853647714 +53.74194392141 14.2070 13.4843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213007_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213007_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:14:27.99 +49:28:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.932 355203489123658496 033.61615616713 +49.46800271294 12.9413 12.4696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213008_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213008_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 213018_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213018_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 213022_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213022_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:42:22.52 +51:49:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.721 451200681114403200 040.59261284153 +51.82060376479 13.6161 13.0074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213025_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213025_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 213034_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213034_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:51:55.23 +52:12:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.958 440748723583628032 042.97835747325 +52.20943908585 13.7951 13.1161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213040_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213040_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 213044_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213044_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 213045_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213045_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 213047_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213047_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 213054_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 213054_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 213060_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213060_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:47:07.24 +49:05:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.293 438646904024651904 041.78011717092 +49.09200871922 13.5289 13.3370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213061_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213061_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 213062_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213062_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:07:38.31 +52:11:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.770 440194118745530880 046.90882282868 +52.18980077098 13.4776 12.7127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213066_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213066_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:05:43.20 +49:12:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.554 358140349102702080 031.42823637112 +49.20503328855 12.1549 11.4433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213071_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213071_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:36:14.76 +57:42:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.908 458111077340756096 039.06180989385 +57.71318149569 13.4204 12.7993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213074_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213074_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 213078_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213078_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 213086_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213086_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:47:43.98 +54:12:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.594 453535734576939776 041.93257070555 +54.20163970236 13.5990 12.6303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213088_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213088_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:33:30.53 +57:34:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.976 458024765678598528 038.37686300486 +57.58271866269 13.0981 12.5589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213093_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213093_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:17:41.87 +56:31:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.275 448010413767267712 049.42546071163 +56.52558325860 13.4826 12.8306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213095_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213095_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 213102_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213102_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 213104_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213104_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:55:26.25 +51:03:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.388 440441032126919808 043.85895609886 +51.05857935121 13.3548 12.5411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213109_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213109_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 213113_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213113_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 213116_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213116_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:28:09.48 +50:55:06.9 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 213123_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213123_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 213135_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213135_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:23:11.39 +55:12:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.782 446948006358984832 050.79738484427 +55.21275919218 13.3966 12.6895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213136_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213136_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:07:43.86 +49:20:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.873 358155948425174656 031.93230330624 +49.33506864898 12.1221 11.3097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213137_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213137_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 213153_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213153_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 213154_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213154_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 213157_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213157_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 213159_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213159_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 213165_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213165_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 213172_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213172_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 213173_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213173_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:26:04.87 +49:46:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.330 441685438770912640 051.51990299892 +49.77399317231 13.2600 12.7070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213174_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213174_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:53:49.21 +53:47:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.283 453242233691177728 043.45513907990 +53.79852583893 13.2851 12.3054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213177_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213177_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 213184_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213184_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:03.23 +57:33:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.022 448878409481190016 056.76390892907 +57.55837879315 12.7742 12.2910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213185_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213185_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:55:30.02 +51:17:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.163 440453706568715904 043.87465552845 +51.29995900018 13.9335 13.2399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213189_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213189_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 213191_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213191_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:05:46.64 +56:38:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 0.324 460021238270908288 046.44419297645 +56.64840743940 13.4476 12.6314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213193_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213193_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 213194_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 213194_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 213197_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213197_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:33:29.99 +57:52:20.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 213199_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213199_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:50:46.66 +57:00:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.057 460621296743076096 042.69546259800 +57.01276866366 14.1451 13.2539 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 213208_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213208_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 213214_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213214_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:51:24.79 +51:20:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.494 440570740139073024 042.85435515585 +51.33733484704 13.8842 13.0119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213220_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213220_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 213222_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213222_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:45:09.84 +58:49:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.536 464089362577527424 041.29026991416 +58.82553120284 13.1406 12.1725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213225_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213225_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 213228_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213228_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:01:54.28 +49:37:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.269 358395641959021184 030.47622131321 +49.62698232048 12.4084 11.5010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213230_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213230_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 213231_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213231_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 213235_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213235_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 213236_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213236_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:14:37.36 +49:27:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.723 355202698849679616 033.65612533464 +49.45125008120 13.1726 12.6375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213239_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213239_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:27:52.55 +50:58:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.704 451652236796832128 036.96867784215 +50.96719499920 13.5740 13.2177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213246_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213246_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 213251_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213251_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 213254_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213254_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:01:51.29 +58:18:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.207 461122536607300608 045.46430951640 +58.31169326554 13.5882 12.8489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213262_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213262_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 213263_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213263_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 213271_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213271_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:21:51.83 +52:20:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.686 443019661769971328 050.46575006241 +52.34645076255 13.9372 13.2526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213272_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213272_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 213273_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213273_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 213275_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213275_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:02:25.60 +49:25:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.615 358390286137689600 030.60546368099 +49.43253721343 12.3330 11.3321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213280_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213280_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 213282_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213282_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:06:33.69 +54:28:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 0.234 447316067876654208 046.64047722009 +54.47294309898 13.9664 13.2188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213286_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213286_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:33:22.98 +58:19:57.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 213287_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213287_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 213289_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213289_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 213292_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213292_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:03:56.64 +48:46:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.120 356814067500010240 030.98483101435 +48.77807538367 12.2854 11.5401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213293_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213293_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 213294_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213294_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 213297_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213297_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:17:52.81 +58:47:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.137 461848764037530112 049.47078783021 +58.78399393169 13.0290 11.9494 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 213298_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213298_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 213306_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213306_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 213310_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213310_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:13:30.83 +58:34:24.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 213315_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213315_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:41:29.28 +58:59:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.951 464203917945587328 040.37063069879 +58.98291620673 13.3990 12.6750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213318_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213318_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:19:40.56 +48:48:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.555 355296088617787776 034.91790362228 +48.80188210657 12.9748 12.1963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213324_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213324_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:05:15.25 +52:36:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.327 440970928011169664 046.31264121620 +52.61662281624 14.2702 13.8062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213338_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213338_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 213344_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213344_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 213350_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213350_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 213354_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 213354_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 213355_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213355_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 213360_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213360_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:10:01.12 +54:10:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.277 447196637724601600 047.50467721753 +54.17675647618 13.7201 12.9381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213365_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213365_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 213369_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213369_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 213375_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213375_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:26.68 +57:42:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.172 448881742368770048 056.86172945332 +57.71565272265 12.8596 12.2878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213376_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213376_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:11:41.52 +49:15:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.770 436391393360975744 047.92324689406 +49.26156338279 13.5517 12.9092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213378_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213378_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:32:24.16 +52:42:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.474 452278477389930752 038.10017599395 +52.70727409418 14.0046 13.3994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213381_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213381_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:15:54.31 +50:58:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.021 442832710434815616 048.97784912175 +50.96929903384 13.8565 13.0890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213385_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213385_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 213387_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213387_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:22:10.81 +53:50:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.499 455550486555029504 035.54398484316 +53.84041748266 13.6752 13.1554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213407_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 213407_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 213417_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213417_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 213424_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213424_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 213435_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213435_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:04:23.53 +50:36:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.927 439760262628246528 046.09735481118 +50.60752279638 13.6656 12.9525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213436_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213436_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 213437_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213437_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 213438_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213438_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 213441_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213441_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 213444_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213444_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 213445_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213445_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:39:48.91 +56:21:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.087 448698433168999936 054.95337438744 +56.36322246422 13.4206 12.7442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213448_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213448_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 213450_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213450_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:37:54.32 +57:07:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.066 448968775589619456 054.47594385120 +57.12512401052 13.3468 12.5843 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 213467_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213467_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 213469_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213469_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 213470_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213470_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 213472_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213472_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 213476_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213476_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 213484_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213484_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 213488_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213488_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 213491_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213491_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 213497_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213497_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 213502_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213502_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 213509_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213509_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:01:56.56 +49:24:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.272 358389319767169920 030.48559837654 +49.41066103128 12.3356 11.8414 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213512_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213512_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 213518_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213518_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 213523_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213523_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 213530_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213530_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 213533_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213533_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 213538_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213538_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 213539_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213539_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:06:10.59 +57:29:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.977 460274813136492544 046.54282215361 +57.49892103003 14.0703 13.2696 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 213540_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213540_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 213545_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213545_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 213546_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 213546_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 213550_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213550_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 213551_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213551_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 213554_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213554_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 213560_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213560_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 213561_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213561_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:37:11.54 +49:58:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.254 450616187604933120 039.29787470844 +49.97242852107 13.6077 13.0841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213568_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213568_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:35:04.82 +49:06:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.157 249310486328721024 053.77023537890 +49.10321473466 13.1872 12.8641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213570_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213570_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 213580_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213580_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:44:28.77 +57:39:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 2.129 448935618447155328 056.12013865023 +57.66528673480 13.2004 12.5948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213582_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213582_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 213585_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213585_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:40:28.10 +51:36:28.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)
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Considering the candidate 213586_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213586_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:48:54.07 +49:10:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 0.944 438603645114422400 042.22560934132 +49.16784009447 13.9666 13.5940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213588_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213588_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 213589_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213589_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 213591_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213591_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 213592_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213592_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 213599_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213599_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:02:29.92 +49:27:19.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)
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Considering the candidate 213601_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213601_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 213602_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213602_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 213610_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213610_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 213611_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213611_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 213618_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213618_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 213627_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213627_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 213631_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213631_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 213633_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 213633_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 213635_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213635_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:48:40.19 +57:48:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.340 460895521815831296 042.16687505144 +57.81221190512 13.7528 13.0941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213636_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213636_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 213641_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213641_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:29:10.82 +48:44:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.957 249242694563930624 052.29434656285 +48.73997669688 13.4429 12.9965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213643_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213643_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 213662_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213662_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:11.76 +57:44:58.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)
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Considering the candidate 213665_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213665_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 213671_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213671_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:10:50.62 +48:44:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.750 355077217084371712 032.71050396571 +48.73871377967 13.2274 12.6750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213674_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213674_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 213680_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213680_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 213681_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213681_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:15:13.18 +48:46:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.327 355133665837568128 033.80488930928 +48.77495012694 13.2908 12.8263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213687_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213687_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 213690_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213690_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 213691_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213691_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 213699_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213699_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 213700_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213700_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:45:32.09 +57:39:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 0.905 448924623330843008 056.38340060267 +57.65794886683 13.2912 12.7555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213703_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213703_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:43:56.78 +52:08:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.541 452709863907551488 040.98580543012 +52.13413089610 14.3356 13.7528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213709_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213709_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:21:22.89 +52:18:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.314 455008667840840576 035.34511276085 +52.30706083971 13.5916 13.0549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213715_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213715_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 213723_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213723_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 213725_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213725_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 213732_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213732_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 213750_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213750_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:44:44.15 +57:48:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.573 448938813902737536 056.18385231203 +57.81499016631 13.1788 12.3947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213756_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213756_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 213757_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213757_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 213759_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213759_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:02:08.66 +49:18:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.794 356886768408100480 030.53537070004 +49.30226419965 12.3145 11.5797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213761_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213761_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:57:58.98 +55:25:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.661 459472238372825088 044.49647123908 +55.42178702258 13.8812 12.8279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213765_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213765_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 213767_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213767_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 213774_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213774_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 213777_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213777_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 213784_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213784_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 213785_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213785_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 213805_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213805_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 213807_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213807_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 213812_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213812_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 213813_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213813_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 213815_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213815_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 213816_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213816_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:10.65 +57:22:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 0.683 448867998480625408 056.54419917796 +57.37869677362 13.1767 12.5113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213817_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213817_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 213818_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213818_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 213820_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213820_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 213826_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213826_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 213838_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213838_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 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 213848_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213848_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 213851_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213851_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 213856_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213856_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 213857_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213857_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 213859_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213859_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 213877_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213877_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 213887_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213887_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 213888_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213888_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:03.79 +57:29:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 0.764 448874767348968064 056.76584492470 +57.49773415938 13.2394 12.7572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213891_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213891_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:18.16 +57:39:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.281 448880402345950592 056.82590306318 +57.65247293642 13.3385 12.6578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213902_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213902_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 213924_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213924_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 213928_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213928_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 213937_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213937_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 213945_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213945_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 213947_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213947_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 213959_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213959_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 213966_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213966_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 213970_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213970_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 213972_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213972_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 213982_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213982_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 213985_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213985_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 213993_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213993_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 213995_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 213995_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 214004_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214004_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 214011_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214011_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:37:25.70 +54:34:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.743 445158899079852160 054.35686864551 +54.58083531429 13.9828 13.2687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214017_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214017_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 214019_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214019_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 214023_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214023_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 214026_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214026_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 214028_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214028_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:03:32.45 +48:59:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 5.649 356820561490539136 030.88303684119 +48.99686984571 12.7103 11.8840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214030_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214030_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 214037_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214037_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 214038_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214038_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 214050_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214050_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 214055_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214055_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:27:36.95 +49:48:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 4.236 441589712540136832 051.90266122943 +49.81306198747 14.0826 13.4548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214056_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214056_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 214063_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214063_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 214070_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214070_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:31:16.16 +50:33:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.963 442011478326708352 052.81672826189 +50.55849437104 13.6832 12.9874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214076_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214076_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 214084_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214084_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 214091_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214091_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 214101_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214101_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:29.69 +57:55:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.029 448946544844057088 056.62421271842 +57.93256690693 13.3365 12.6881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214123_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214123_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 214125_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214125_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 214126_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214126_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 214141_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214141_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:46:30.01 +57:26:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.210 448868754394823296 056.62495956326 +57.43997223327 13.3783 12.8976 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214147_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214147_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 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 214158_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214158_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 214165_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214165_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 214169_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214169_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:06:29.65 +48:45:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 3.755 358110662290036864 031.62203690057 +48.76159389806 13.0165 12.3186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214173_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214173_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 214180_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214180_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:14.13 +57:36:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 2.172 448878615639579648 056.80926220257 +57.60723911655 13.6327 13.1169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214187_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214187_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:47:07.63 +57:47:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 0.902 448930086529105152 056.78224972371 +57.79741795347 13.3973 12.7667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214188_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214188_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 214192_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214192_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 214197_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214197_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 214201_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214201_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 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 214203_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214203_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 214208_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214208_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 214214_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214214_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 214215_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214215_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 214218_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214218_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 214222_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214222_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 214223_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214223_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 214225_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214225_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 214227_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214227_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 214234_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214234_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 214239_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214239_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 214241_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214241_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:45:25.96 +57:30:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.323 448918369858550144 056.35808571729 +57.50314360605 13.6100 13.1266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214252_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214252_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 214259_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214259_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 214271_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214271_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 214272_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214272_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 214278_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214278_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 214282_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214282_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 214285_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214285_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 214287_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214287_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 214292_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214292_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 214308_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214308_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 214312_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214312_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 214321_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214321_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 214333_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214333_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 214340_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214340_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 214366_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 214366_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 10331_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 10331_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:58:58.30 +58:33:20.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)
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Considering the candidate 69806_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 69806_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 101918_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 101918_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 168323_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 168323_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 97368_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 97368_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 148139_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 148139_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 178097_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 178097_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:06:00.40 +50:19:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.974 358491509927468160 031.50006193358 +50.32648962984 12.9139 12.2197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 164749_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 164749_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:18:18.57 +49:41:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.288 355546845989193728 034.57770675759 +49.69079703979 12.9635 12.5681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 60460_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 60460_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 109364_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 109364_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 53156_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 53156_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 113964_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 113964_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 71211_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 71211_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 200966_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 200966_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:44:51.85 +57:19:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.820 448846553702525312 056.21612453819 +57.32294329168 12.6928 12.1372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65107_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 65107_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 200538_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 200538_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:42:19.35 +57:25:02.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)
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Considering the candidate 86656_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 86656_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 165397_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 165397_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 184652_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 184652_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:58:52.20 +50:37:36.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)
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Considering the candidate 57608_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 57608_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 11807_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 11807_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 200010_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 200010_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:33:00.14 +56:51:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.183 448639128259019776 053.25010367359 +56.85148096376 13.2870 12.4314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 199910_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 199910_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:43:34.11 +57:00:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.069 448833020266333696 055.89266717467 +57.00538625708 12.9757 12.2606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82135_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 82135_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 107170_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 107170_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 54386_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 54386_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 77474_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 77474_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 47709_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 47709_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 108361_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 108361_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 19789_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 19789_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 51319_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 51319_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 156448_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 156448_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 182631_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 182631_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 32199_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 32199_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:13:48.56 +56:56:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.912 448072364375201920 048.45327600570 +56.94316062858 12.1393 10.5560 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116633_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 116633_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:52:54.17 +52:37:14.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)
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Considering the candidate 71790_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 71790_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 105309_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 105309_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 66917_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 66917_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 78022_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 78022_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 03176_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 03176_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 113372_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
Preparing report for the candidate 113372_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
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Considering the candidate 142862_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 142862_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 02:19:14.40 +51:15:28.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203687_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 203687_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:36:35.08 +58:09:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.050 449846117148589440 054.14530106496 +58.16604838873 13.0061 12.4566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 76844_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 76844_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
**** FOUND 03:30:48.86 +53:53:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 2.935 443579244469162880 052.70226109060 +53.88978789363 13.8055 12.9730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 28133_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 28133_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 38437_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013
The candidate 38437_Per-01-Q2b1x1_2026-02-26_22-27-34_20.00sec_-15.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 19s
make_report_in_HTML.sh TOTAL: 166s
Prepared the HTML report for the field Per-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:19:14.40 +51:15:28.2
03:46:19.19 +57:47:36.6
02:19:55.81 +53:28:08.8
02:47:28.32 +53:09:14.3
02:21:34.90 +53:10:06.9
02:43:37.56 +53:05:01.6
02:57:02.96 +52:43:56.5
02:22:56.64 +51:34:15.5
02:32:11.60 +49:54:43.5
02:56:42.34 +50:33:28.4
03:41:25.10 +56:55:32.8
01:56:32.09 +57:23:06.0
02:03:22.79 +49:39:05.0
01:59:11.99 +51:55:30.9
02:03:54.56 +49:11:54.6
02:01:45.17 +58:24:19.7
03:43:50.82 +56:50:37.1
01:57:48.22 +57:18:36.4
01:54:31.93 +56:47:31.8
01:53:33.90 +57:43:27.6
01:57:17.91 +56:32:02.5
01:54:22.12 +57:13:18.8
01:53:50.28 +58:01:22.9
01:58:23.03 +55:54:35.4
01:57:10.61 +57:18:12.5
02:01:27.67 +50:11:24.2
02:01:37.10 +58:22:38.8
01:53:54.96 +56:44:08.9
01:58:21.88 +58:00:55.1
01:55:01.43 +57:05:05.8
02:00:44.09 +58:16:23.8
02:01:26.14 +56:17:43.5
01:59:58.86 +57:13:28.3
01:59:37.71 +58:21:54.2
01:56:10.98 +55:30:13.3
01:53:33.64 +58:23:36.9
01:55:47.67 +55:57:51.4
01:58:39.94 +58:15:34.9
01:57:25.67 +55:41:39.6
01:56:42.84 +57:03:00.6
01:57:31.19 +58:04:39.1
02:01:39.48 +51:08:45.5
01:53:17.83 +57:14:43.9
02:00:30.82 +58:23:14.7
01:58:23.60 +58:14:23.2
02:02:29.09 +57:55:02.1
01:54:45.11 +57:29:50.1
01:55:49.17 +57:55:52.4
01:58:32.91 +56:30:56.7
01:55:08.51 +56:58:20.0
01:59:54.17 +57:34:41.1
01:56:28.02 +58:12:14.2
01:54:13.49 +57:32:11.1
01:53:46.47 +57:10:59.6
01:57:01.66 +56:14:15.7
02:00:21.48 +58:23:30.3
02:04:05.89 +49:42:42.5
02:02:45.48 +48:39:18.7
01:53:22.51 +56:41:49.4
02:30:08.24 +57:48:49.6
02:45:18.56 +57:37:52.4
02:01:26.00 +50:25:11.4
02:02:51.59 +58:02:51.1
03:15:40.81 +51:11:16.4
02:42:52.38 +48:55:46.4
02:06:19.70 +48:49:32.4
02:32:46.55 +56:29:27.8
03:12:59.67 +55:44:11.9
02:18:31.15 +56:04:11.5
02:42:06.27 +55:53:27.7
02:18:51.55 +55:21:05.4
02:41:07.96 +55:12:59.9
02:47:19.78 +55:04:00.2
02:38:23.71 +55:07:25.8
02:50:25.41 +54:45:23.3
02:50:00.08 +53:38:56.3
########### Completed Per-01-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
02:19:14.40 +51:15:28.2
01:56:32.09 +57:23:06.0
02:03:22.79 +49:39:05.0
01:59:11.99 +51:55:30.9
02:03:54.56 +49:11:54.6
02:01:45.17 +58:24:19.7
03:43:50.82 +56:50:37.1
01:57:48.22 +57:18:36.4
01:54:31.93 +56:47:31.8
01:53:33.90 +57:43:27.6
01:57:17.91 +56:32:02.5
01:54:22.12 +57:13:18.8
01:53:50.28 +58:01:22.9
01:58:23.03 +55:54:35.4
01:57:10.61 +57:18:12.5
02:01:27.67 +50:11:24.2
02:01:37.10 +58:22:38.8
01:53:54.96 +56:44:08.9
01:58:21.88 +58:00:55.1
01:55:01.43 +57:05:05.8
02:00:44.09 +58:16:23.8
02:01:26.14 +56:17:43.5
01:59:58.86 +57:13:28.3
01:59:37.71 +58:21:54.2
01:56:10.98 +55:30:13.3
01:53:33.64 +58:23:36.9
01:55:47.67 +55:57:51.4
01:58:39.94 +58:15:34.9
01:57:25.67 +55:41:39.6
01:56:42.84 +57:03:00.6
01:57:31.19 +58:04:39.1
02:01:39.48 +51:08:45.5
01:53:17.83 +57:14:43.9
02:00:30.82 +58:23:14.7
01:58:23.60 +58:14:23.2
02:02:29.09 +57:55:02.1
01:54:45.11 +57:29:50.1
01:55:49.17 +57:55:52.4
01:58:32.91 +56:30:56.7
01:55:08.51 +56:58:20.0
01:59:54.17 +57:34:41.1
01:56:28.02 +58:12:14.2
01:54:13.49 +57:32:11.1
01:53:46.47 +57:10:59.6
01:57:01.66 +56:14:15.7
02:00:21.48 +58:23:30.3
02:04:05.89 +49:42:42.5
02:02:45.48 +48:39:18.7
01:53:22.51 +56:41:49.4
02:30:08.24 +57:48:49.6
02:45:18.56 +57:37:52.4
02:01:26.00 +50:25:11.4
02:02:51.59 +58:02:51.1
03:15:40.81 +51:11:16.4
02:42:52.38 +48:55:46.4
02:06:19.70 +48:49:32.4
02:41:07.96 +55:12:59.9
02:19:55.81 +53:28:08.8
02:32:11.60 +49:54:43.5
02:50:00.08 +53:38:56.3
02:22:56.64 +51:34:15.5
02:43:37.56 +53:05:01.6
03:12:59.67 +55:44:11.9
02:47:19.78 +55:04:00.2
02:42:06.27 +55:53:27.7
02:47:28.32 +53:09:14.3
02:18:31.15 +56:04:11.5
02:50:25.41 +54:45:23.3
02:32:46.55 +56:29:27.8
02:21:34.90 +53:10:06.9
03:41:25.10 +56:55:32.8
02:56:42.34 +50:33:28.4
02:38:23.71 +55:07:25.8
02:18:51.55 +55:21:05.4
03:46:19.19 +57:47:36.6
02:57:02.96 +52:43:56.5
###################################################################################
02:19:14.40 +51:15:28.2 -- not an asteroid (will add it to exclusion list)
01:56:32.09 +57:23:06.0 -- not an asteroid (will add it to exclusion list)
02:03:22.79 +49:39:05.0 -- not an asteroid (will add it to exclusion list)
01:59:11.99 +51:55:30.9 -- not an asteroid (will add it to exclusion list)
02:03:54.56 +49:11:54.6 -- not an asteroid (will add it to exclusion list)
02:01:45.17 +58:24:19.7 -- not an asteroid (will add it to exclusion list)
03:43:50.82 +56:50:37.1 -- not an asteroid (will add it to exclusion list)
01:57:48.22 +57:18:36.4 -- not an asteroid (will add it to exclusion list)
01:54:31.93 +56:47:31.8 -- not an asteroid (will add it to exclusion list)
01:53:33.90 +57:43:27.6 -- not an asteroid (will add it to exclusion list)
01:57:17.91 +56:32:02.5 -- not an asteroid (will add it to exclusion list)
01:54:22.12 +57:13:18.8 -- not an asteroid (will add it to exclusion list)
01:53:50.28 +58:01:22.9 -- not an asteroid (will add it to exclusion list)
01:58:23.03 +55:54:35.4 -- not an asteroid (will add it to exclusion list)
01:57:10.61 +57:18:12.5 -- not an asteroid (will add it to exclusion list)
02:01:27.67 +50:11:24.2 -- not an asteroid (will add it to exclusion list)
02:01:37.10 +58:22:38.8 -- not an asteroid (will add it to exclusion list)
01:53:54.96 +56:44:08.9 -- not an asteroid (will add it to exclusion list)
01:58:21.88 +58:00:55.1 -- not an asteroid (will add it to exclusion list)
01:55:01.43 +57:05:05.8 -- not an asteroid (will add it to exclusion list)
02:00:44.09 +58:16:23.8 -- not an asteroid (will add it to exclusion list)
02:01:26.14 +56:17:43.5 -- not an asteroid (will add it to exclusion list)
01:59:58.86 +57:13:28.3 -- not an asteroid (will add it to exclusion list)
01:59:37.71 +58:21:54.2 -- not an asteroid (will add it to exclusion list)
01:56:10.98 +55:30:13.3 -- not an asteroid (will add it to exclusion list)
01:53:33.64 +58:23:36.9 -- not an asteroid (will add it to exclusion list)
01:55:47.67 +55:57:51.4 -- not an asteroid (will add it to exclusion list)
01:58:39.94 +58:15:34.9 -- not an asteroid (will add it to exclusion list)
01:57:25.67 +55:41:39.6 -- not an asteroid (will add it to exclusion list)
01:56:42.84 +57:03:00.6 -- not an asteroid (will add it to exclusion list)
01:57:31.19 +58:04:39.1 -- not an asteroid (will add it to exclusion list)
02:01:39.48 +51:08:45.5 -- not an asteroid (will add it to exclusion list)
01:53:17.83 +57:14:43.9 -- not an asteroid (will add it to exclusion list)
02:00:30.82 +58:23:14.7 -- not an asteroid (will add it to exclusion list)
01:58:23.60 +58:14:23.2 -- not an asteroid (will add it to exclusion list)
02:02:29.09 +57:55:02.1 -- not an asteroid (will add it to exclusion list)
01:54:45.11 +57:29:50.1 -- not an asteroid (will add it to exclusion list)
01:55:49.17 +57:55:52.4 -- not an asteroid (will add it to exclusion list)
01:58:32.91 +56:30:56.7 -- not an asteroid (will add it to exclusion list)
01:55:08.51 +56:58:20.0 -- not an asteroid (will add it to exclusion list)
01:59:54.17 +57:34:41.1 -- not an asteroid (will add it to exclusion list)
01:56:28.02 +58:12:14.2 -- not an asteroid (will add it to exclusion list)
01:54:13.49 +57:32:11.1 -- not an asteroid (will add it to exclusion list)
01:53:46.47 +57:10:59.6 -- not an asteroid (will add it to exclusion list)
01:57:01.66 +56:14:15.7 -- not an asteroid (will add it to exclusion list)
02:00:21.48 +58:23:30.3 -- not an asteroid (will add it to exclusion list)
02:04:05.89 +49:42:42.5 -- not an asteroid (will add it to exclusion list)
02:02:45.48 +48:39:18.7 -- not an asteroid (will add it to exclusion list)
01:53:22.51 +56:41:49.4 -- not an asteroid (will add it to exclusion list)
02:30:08.24 +57:48:49.6 -- not an asteroid (will add it to exclusion list)
02:45:18.56 +57:37:52.4 -- not an asteroid (will add it to exclusion list)
02:01:26.00 +50:25:11.4 -- not an asteroid (will add it to exclusion list)
02:02:51.59 +58:02:51.1 -- not an asteroid (will add it to exclusion list)
03:15:40.81 +51:11:16.4 -- not an asteroid (will add it to exclusion list)
02:42:52.38 +48:55:46.4 -- not an asteroid (will add it to exclusion list)
02:06:19.70 +48:49:32.4 -- not an asteroid (will add it to exclusion list)
02:41:07.96 +55:12:59.9 -- not an asteroid (will add it to exclusion list)
02:19:55.81 +53:28:08.8 -- not an asteroid (will add it to exclusion list)
02:32:11.60 +49:54:43.5 -- not an asteroid (will add it to exclusion list)
02:50:00.08 +53:38:56.3 -- not an asteroid (will add it to exclusion list)
02:22:56.64 +51:34:15.5 -- not an asteroid (will add it to exclusion list)
02:43:37.56 +53:05:01.6 -- not an asteroid (will add it to exclusion list)
03:12:59.67 +55:44:11.9 -- not an asteroid (will add it to exclusion list)
02:47:19.78 +55:04:00.2 -- not an asteroid (will add it to exclusion list)
02:42:06.27 +55:53:27.7 -- not an asteroid (will add it to exclusion list)
02:47:28.32 +53:09:14.3 -- not an asteroid (will add it to exclusion list)
02:18:31.15 +56:04:11.5 -- not an asteroid (will add it to exclusion list)
02:50:25.41 +54:45:23.3 -- not an asteroid (will add it to exclusion list)
02:32:46.55 +56:29:27.8 -- not an asteroid (will add it to exclusion list)
02:21:34.90 +53:10:06.9 -- not an asteroid (will add it to exclusion list)
03:41:25.10 +56:55:32.8 -- not an asteroid (will add it to exclusion list)
02:56:42.34 +50:33:28.4 -- not an asteroid (will add it to exclusion list)
02:38:23.71 +55:07:25.8 -- not an asteroid (will add it to exclusion list)
02:18:51.55 +55:21:05.4 -- not an asteroid (will add it to exclusion list)
03:46:19.19 +57:47:36.6 -- not an asteroid (will add it to exclusion list)
02:57:02.96 +52:43:56.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:53:17.83 +57:14:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:22.51 +56:41:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:33.64 +58:23:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:33.90 +57:43:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:46.47 +57:10:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:50.28 +58:01:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:54.96 +56:44:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:13.49 +57:32:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:22.12 +57:13:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:31.93 +56:47:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:45.11 +57:29:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:01.43 +57:05:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:08.51 +56:58:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:47.67 +55:57:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:49.17 +57:55:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:10.98 +55:30:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:28.02 +58:12:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:32.09 +57:23:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:42.84 +57:03:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:01.66 +56:14:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:10.61 +57:18:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:17.91 +56:32:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:25.67 +55:41:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:31.19 +58:04:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:48.22 +57:18:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:21.88 +58:00:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:23.03 +55:54:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:23.60 +58:14:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:32.91 +56:30:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:39.94 +58:15:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:11.99 +51:55:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:37.71 +58:21:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:54.17 +57:34:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:58.86 +57:13:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:21.48 +58:23:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:30.82 +58:23:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:44.09 +58:16:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:26.00 +50:25:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:26.14 +56:17:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:27.67 +50:11:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:37.10 +58:22:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:39.48 +51:08:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:45.17 +58:24:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:29.09 +57:55:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:45.48 +48:39:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:51.59 +58:02:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:22.79 +49:39:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:54.56 +49:11:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:05.89 +49:42:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:19.70 +48:49:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:31.15 +56:04:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:51.55 +55:21:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:14.40 +51:15:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:55.81 +53:28:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:34.90 +53:10:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:56.64 +51:34:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:08.24 +57:48:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:11.60 +49:54:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:46.55 +56:29:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:23.71 +55:07:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:41:07.96 +55:12:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:42:06.27 +55:53:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:42:52.38 +48:55:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:43:37.56 +53:05:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:45:18.56 +57:37:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:47:19.78 +55:04:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:47:28.32 +53:09:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:50:00.08 +53:38:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:50:25.41 +54:45:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:42.34 +50:33:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:02.96 +52:43:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:12:59.67 +55:44:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:40.81 +51:11:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:25.10 +56:55:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:50.82 +56:50:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:19.19 +57:47:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:53:17.83 +57:14:43.9 -- not a known variable star
01:53:22.51 +56:41:49.4 -- a known variable star
01:53:33.64 +58:23:36.9 -- not a known variable star
01:53:33.90 +57:43:27.6 -- a known variable star
01:53:46.47 +57:10:59.6 -- not a known variable star
01:53:50.28 +58:01:22.9 -- a known variable star
01:53:54.96 +56:44:08.9 -- not a known variable star
01:54:13.49 +57:32:11.1 -- a known variable star
01:54:22.12 +57:13:18.8 -- a known variable star
01:54:31.93 +56:47:31.8 -- not a known variable star
01:54:45.11 +57:29:50.1 -- not a known variable star
01:55:01.43 +57:05:05.8 -- a known variable star
01:55:08.51 +56:58:20.0 -- not a known variable star
01:55:47.67 +55:57:51.4 -- not a known variable star
01:55:49.17 +57:55:52.4 -- not a known variable star
01:56:10.98 +55:30:13.3 -- not a known variable star
01:56:28.02 +58:12:14.2 -- not a known variable star
01:56:32.09 +57:23:06.0 -- a known variable star
01:56:42.84 +57:03:00.6 -- not a known variable star
01:57:01.66 +56:14:15.7 -- not a known variable star
01:57:10.61 +57:18:12.5 -- not a known variable star
01:57:17.91 +56:32:02.5 -- not a known variable star
01:57:25.67 +55:41:39.6 -- not a known variable star
01:57:31.19 +58:04:39.1 -- not a known variable star
01:57:48.22 +57:18:36.4 -- a known variable star
01:58:21.88 +58:00:55.1 -- a known variable star
01:58:23.03 +55:54:35.4 -- not a known variable star
01:58:23.60 +58:14:23.2 -- not a known variable star
01:58:32.91 +56:30:56.7 -- a known variable star
01:58:39.94 +58:15:34.9 -- a known variable star
01:59:11.99 +51:55:30.9 -- not a known variable star
01:59:37.71 +58:21:54.2 -- not a known variable star
01:59:54.17 +57:34:41.1 -- not a known variable star
01:59:58.86 +57:13:28.3 -- a known variable star
02:00:21.48 +58:23:30.3 -- not a known variable star
02:00:30.82 +58:23:14.7 -- not a known variable star
02:00:44.09 +58:16:23.8 -- not a known variable star
02:01:26.00 +50:25:11.4 -- not a known variable star
02:01:26.14 +56:17:43.5 -- not a known variable star
02:01:27.67 +50:11:24.2 -- not a known variable star
02:01:37.10 +58:22:38.8 -- not a known variable star
02:01:39.48 +51:08:45.5 -- not a known variable star
02:01:45.17 +58:24:19.7 -- not a known variable star
02:02:29.09 +57:55:02.1 -- not a known variable star
02:02:45.48 +48:39:18.7 -- not a known variable star
02:02:51.59 +58:02:51.1 -- not a known variable star
02:03:22.79 +49:39:05.0 -- not a known variable star
02:03:54.56 +49:11:54.6 -- not a known variable star
02:04:05.89 +49:42:42.5 -- not a known variable star
02:06:19.70 +48:49:32.4 -- a known variable star
02:18:31.15 +56:04:11.5 -- a known variable star
02:18:51.55 +55:21:05.4 -- a known variable star
02:19:14.40 +51:15:28.2 -- a known variable star
02:19:55.81 +53:28:08.8 -- a known variable star
02:21:34.90 +53:10:06.9 -- a known variable star
02:22:56.64 +51:34:15.5 -- a known variable star
02:30:08.24 +57:48:49.6 -- not a known variable star
02:32:11.60 +49:54:43.5 -- a known variable star
02:32:46.55 +56:29:27.8 -- a known variable star
02:38:23.71 +55:07:25.8 -- a known variable star
02:41:07.96 +55:12:59.9 -- a known variable star
02:42:06.27 +55:53:27.7 -- a known variable star
02:42:52.38 +48:55:46.4 -- not a known variable star
02:43:37.56 +53:05:01.6 -- a known variable star
02:45:18.56 +57:37:52.4 -- not a known variable star
02:47:19.78 +55:04:00.2 -- a known variable star
02:47:28.32 +53:09:14.3 -- not a known variable star
02:50:00.08 +53:38:56.3 -- a known variable star
02:50:25.41 +54:45:23.3 -- a known variable star
02:56:42.34 +50:33:28.4 -- a known variable star
02:57:02.96 +52:43:56.5 -- a known variable star
03:12:59.67 +55:44:11.9 -- a known variable star
03:15:40.81 +51:11:16.4 -- a known variable star
03:41:25.10 +56:55:32.8 -- not a known variable star
03:43:50.82 +56:50:37.1 -- a known variable star
03:46:19.19 +57:47:36.6 -- not a known variable star
Found 43 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
76 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 76 (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)2461098.68536862 -observatory 500
23:26:24.30 -00:23:24.0 Mercury (1.2mag)
23:27:34.85 -05:00:13.5 Venus (-3.9mag)
21:58:10.75 -13:33:23.9 Mars (1.1mag)
07:05:05.10 +22:56:16.5 Jupiter (-2.5mag)
00:07:34.86 -01:30:10.6 Saturn (1.0mag)
03:40:21.75 +19:23:03.1 Uranus (5.7mag)
00:04:19.49 -00:57:22.5 Neptune (7.8mag)
20:29:43.33 -22:58:11.7 Pluto (14.5mag)
06:59:56.03 +27:05:20.7 Moon (-11.3mag)
-rw-r--r-- 1 apache apache 362 Feb 27 01:54 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461098.68536862:
07:05:00.66 +22:56:27.4 Io (5.4mag)
07:04:57.71 +22:56:27.1 Europa (5.6mag)
07:04:45.84 +22:56:46.9 Ganymede (5.0mag)
07:05:32.41 +22:55:17.0 Callisto (6.2mag)
07:08:33.58 +23:10:12.7 Himalia (15.1mag)
07:05:03.15 +22:56:17.0 Thebe (15.9mag)
07:07:56.02 +23:21:42.1 Elara (17.0mag)
07:00:54.42 +24:01:35.4 Pasiphae (17.1mag)
07:14:04.79 +22:45:42.9 Carme (18.1mag)
00:07:34.69 -01:29:50.9 Titan (8.8mag)
00:07:40.39 -01:30:06.3 Rhea (10.1mag)
00:07:42.59 -01:30:57.5 Iapetus (11.5mag)
00:07:49.60 -01:30:17.5 Hyperion (14.8mag)
00:09:37.86 -01:17:26.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 27 01:54 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461098.68536862:
09:27:45.25 +24:03:39.6 JWST
20:41:00.12 -14:32:32.9 Chandra
07:48:15.27 -25:23:32.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 27 01:54 spacecraft.txt
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Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461098.68536862 at 500
17:09:26.61 -11:06:31.7 17.4mag 10P/Tempel 2
03:42:26.53 +29:15:48.6 18.0mag 123P/West-Hartley
04:49:07.96 +19:34:50.0 0.0mag 124P/Mrkos
21:36:34.14 -06:11:14.6 22.0mag 141P/Machholz
01:32:23.42 +13:19:12.1 17.7mag 145P/Shoemaker-Levy 5
10:58:09.83 +31:05:20.2 18.0mag 164P/Christensen
09:30:24.22 -33:36:10.0 18.0mag 195P/Hill
15:50:58.18 -06:05:28.7 19.5mag 210P/Christensen
18:39:59.19 -21:05:06.1 17.2mag 218P/LINEAR
16:29:51.97 -18:01:45.7 15.2mag 235P/LINEAR
04:03:50.34 +28:38:25.7 17.9mag 240P/NEAT
15:22:46.85 +06:17:27.1 14.9mag 24P/Schaumasse
11:21:26.10 -03:14:49.7 17.3mag 29P/Schwassmann-Wachmann 1
07:03:35.54 +27:25:31.4 19.6mag 407P/PanSTARRS-Fuls
17:15:13.62 -11:15:44.0 17.6mag 40P/Vaisala 1
10:58:52.93 -08:32:42.2 16.6mag 43P/Wolf-Harrington
13:25:16.63 -06:03:09.0 20.2mag 489P/Denning
04:38:23.39 +48:10:27.6 17.8mag 493P/2024 Q2 (LONEOS)
06:06:54.42 +46:34:53.9 17.6mag 63P/Wild 1
23:24:40.23 -01:11:28.3 16.2mag 78P/Gehrels 2
20:20:16.23 -21:30:26.1 14.9mag 88P/Howell
20:47:39.90 -28:44:58.7 0.0mag P/2010 H3 (SOHO)
15:30:09.95 -29:23:56.4 18.6mag P/2023 S1 (PanSTARRS)
04:44:07.81 -72:18:24.1 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:11.98 +31:13:43.9 18.2mag C/2017 K2 (PanSTARRS)
20:09:19.82 -65:21:51.4 18.1mag C/2020 V2 (ZTF)
17:23:40.97 +04:53:34.5 16.3mag C/2021 G2 (ATLAS)
03:39:50.35 +24:43:10.0 15.8mag C/2022 N2 (PanSTARRS)
09:06:33.66 +30:12:53.2 15.3mag C/2022 QE78 (ATLAS)
08:34:13.67 -05:56:15.8 16.7mag C/2022 R6 (PanSTARRS)
23:59:23.34 +48:40:07.0 18.0mag C/2023 C2 (ATLAS)
09:45:39.03 -20:00:31.9 17.5mag C/2023 F3 (ATLAS)
20:44:35.01 +61:15:42.7 17.3mag C/2023 H5 (Lemmon)
19:34:57.59 -03:26:25.7 16.0mag C/2023 R1 (PANSTARRS)
02:50:43.27 +35:38:45.0 18.5mag C/2023 RS61 (PanSTARRS)
21:09:32.46 +81:28:24.3 18.0mag C/2023 X2 (Lemmon)
06:32:22.57 +63:54:11.1 17.4mag C/2024 A1 (ATLAS)
02:30:33.63 -17:44:36.2 11.5mag C/2024 E1 (Wierzchos)
11:40:56.04 -01:36:52.8 18.1mag C/2024 G2 (ATLAS)
19:33:04.26 +00:49:54.3 18.9mag C/2024 G4 (PanSTARRS)
16:36:54.50 -01:02:41.7 17.7mag C/2024 G6 (ATLAS)
19:56:52.06 +04:11:38.1 15.5mag C/2024 J3 (ATLAS)
02:50:02.23 -30:37:36.7 15.4mag C/2024 T5 (ATLAS)
16:09:38.50 -60:08:00.2 15.7mag C/2025 A6 (Lemmon)
04:50:04.68 +60:16:56.5 16.7mag C/2025 J1 (Borisov)
15:52:32.12 -08:33:39.2 14.7mag C/2025 L1 (ATLAS)
02:24:43.29 -19:47:15.2 16.8mag C/2025 Q3 (ATLAS)
02:15:58.26 +17:45:09.7 21.3mag C/2025 R2 (SWAN)
22:22:37.88 +17:48:16.8 16.1mag C/2025 R3 (PANSTARRS)
21:51:16.53 -17:53:57.8 22.1mag C/2025 T1 (ATLAS)
02:55:12.26 -18:05:39.3 18.1mag C/2026 A1 (MAPS)
21:21:44.04 +23:07:54.8 17.0mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 27 01:55 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
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
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
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
09:27:23.49 -32:00:30.90 SN 2023kuy 2026-01-21.16 15.43
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
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
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
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
-rw-r--r-- 1 apache apache 5.7K Feb 27 01:54 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
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
-rw-r--r-- 1 apache apache 187K Feb 27 01:54 tocp_transients_list.txt