This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 12.46 03:42:34.79 +41:05:34.3
154.37687 -11.10131 galactic Per Second-epoch detections are separated by 2.1" 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 225133703100028288 | 03:42:35.45 +41:05:34.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 34.79 +41 05 34.3 12.5 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 225133703100028288,2461119.5885,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 225133703100028288 20260320.0885 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:34.79 +41:05:34.3 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 41 34.73 +41 05 57.2 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
Gaia DR3 237053336859000064,2461119.5885,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 237053336859000064 20260320.0885 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:34.73 +41:05:57.2 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 11.40 03:47:51.39 +42:24:54.6
154.32415 -9.45385 galactic Per Second-epoch detections are separated by 3.0" 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 | Gaia DR3 231228605292032512 | 03:47:52.05 +42:24:53.1 (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 03 20.0885* 03 47 51.39 +42 24 54.6 11.4 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 231228605292032512,2461119.5885,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 231228605292032512 20260320.0885 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:51.39 +42:24:54.6 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 51 17.02 +33 02 15.5 10.6 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
RX Per,2461119.5885,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RX Per 20260320.0885 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:17.02 +33:02:15.5 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 04 29 15.07 +39 33 44.0 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
GY Per,2461119.5885,10.18,0.05,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
GY Per 20260320.0885 10.18CV 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:15.07 +39:33:44.0 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 04 15 40.68 +35 31 59.3 11.6 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
NSV 1531,2461119.5885,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 1531 20260320.0885 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:40.68 +35:31:59.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 45 20.83 +41 42 39.4 14.3 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
target,2461119.5885,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:20.83 +41:42:39.4 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 19.67 +39 27 33.0 14.2 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
target,2461119.5885,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:19.67 +39:27:33.0 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 14.12 03:47:32.26 +42:45:41.3
154.05769 -9.22096 galactic Per Second-epoch detections are separated by 3.3" 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 | target | 03:47:32.26 +42:45:41.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 47 32.26 +42 45 41.3 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
target,2461119.5885,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:32.26 +42:45:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 14.10 03:41:21.09 +41:02:18.0
154.22482 -11.28659 galactic Per Second-epoch detections are separated by 7.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J055.3447+41.0359 | 03:41:21.09 +41:02:18.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) 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 03 20.0885* 03 41 21.09 +41 02 18.0 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
ATO J055.3447+41.0359,2461119.5885,14.10,0.05,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 J055.3447+41.0359 20260320.0885 14.10CV 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:21.09 +41:02:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.88 03:44:17.38 +42:09:08.9
153.96695 -10.07053 galactic Per Second-epoch detections are separated by 3.3" 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 | Gaia DR3 243216404470946688 | 03:44:17.44 +42:08:31.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 44 17.38 +42 09 08.9 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 243216404470946688,2461119.5885,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 243216404470946688 20260320.0885 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:17.38 +42:09:08.9 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.93 03:43:38.12 +41:29:24.6
154.28605 -10.66633 galactic Per Second-epoch detections are separated by 5.9" 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 | target | 03:43:38.12 +41:29:24.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 38.12 +41 29 24.6 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
target,2461119.5885,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:38.12 +41:29:24.6 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.86 03:44:40.22 +41:24:56.8
154.48783 -10.60455 galactic Per Second-epoch detections are separated by 2.1" 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 | target | 03:44:40.22 +41:24:56.8 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 44 40.22 +41 24 56.8 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
target,2461119.5885,13.86,0.05,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
target 20260320.0885 13.86CV 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:40.22 +41:24:56.8 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 47 30.37 +42 27 07.4 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
target,2461119.5885,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:30.37 +42:27:07.4 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 41 58.62 +40 15 22.1 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
target,2461119.5885,13.95,0.05,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
target 20260320.0885 13.95CV 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:58.62 +40:15:22.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.93 03:47:52.39 +42:49:22.9
154.06716 -9.13442 galactic Per Second-epoch detections are separated by 0.9" 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 J056.9713+42.8232 | 03:47:52.39 +42:49:22.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 47 52.39 +42 49 22.9 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
ATO J056.9713+42.8232,2461119.5885,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J056.9713+42.8232 20260320.0885 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:52.39 +42:49:22.9 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 47 29.73 +42 33 17.4 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
target,2461119.5885,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:29.73 +42:33:17.4 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.76 03:43:14.80 +40:54:09.8
154.59736 -11.17328 galactic Per Second-epoch detections are separated by 2.3" and 3.3 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 | target | 03:43:14.80 +40:54:09.8 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 14.80 +40 54 09.8 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
target,2461119.5885,13.76,0.05,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
target 20260320.0885 13.76CV 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:14.80 +40:54:09.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 13.37 +39 03 41.7 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
target,2461119.5885,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:13.37 +39:03:41.7 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 20.92 +40 30 52.2 13.7 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
target,2461119.5885,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:20.92 +40:30:52.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 46 32.64 +41 30 32.9 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
target,2461119.5885,13.79,0.05,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
target 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:32.64 +41:30:32.9 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 47.44 +39 52 37.5 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
target,2461119.5885,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:47.44 +39:52:37.5 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.70 03:42:54.25 +42:21:53.7
153.62892 -10.06148 galactic Per Second-epoch detections are separated by 2.1" 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 | target | 03:42:54.25 +42:21:53.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 54.25 +42 21 53.7 13.7 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
target,2461119.5885,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:54.25 +42:21:53.7 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.86 03:41:16.75 +41:38:03.5
153.84208 -10.82371 galactic Per Second-epoch detections are separated by 1.7" 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 | target | 03:41:16.75 +41:38:03.5 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 41 16.75 +41 38 03.5 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
target,2461119.5885,13.86,0.05,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
target 20260320.0885 13.86CV 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:16.75 +41:38:03.5 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 18.74 +42 23 14.7 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
target,2461119.5885,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:18.74 +42:23:14.7 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.73 03:42:53.63 +41:49:10.8
153.96836 -10.49247 galactic Per Second-epoch detections are separated by 2.1" 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 | ATO J055.7237+41.8203 | 03:42:53.63 +41:49:10.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 53.63 +41 49 10.8 13.7 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 J055.7237+41.8203,2461119.5885,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J055.7237+41.8203 20260320.0885 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:53.63 +41:49:10.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.71 03:46:25.35 +42:33:38.1
154.02285 -9.50593 galactic Per Second-epoch detections are separated by 1.1" 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 J056.6076+42.5539 | 03:46:25.35 +42:33:38.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 46 25.35 +42 33 38.1 13.7 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 J056.6076+42.5539,2461119.5885,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J056.6076+42.5539 20260320.0885 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:25.35 +42:33:38.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.59 03:43:21.08 +42:17:26.3
153.74151 -10.06914 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 | target | 03:43:21.08 +42:17:26.3 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 21.08 +42 17 26.3 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
target,2461119.5885,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:21.08 +42:17:26.3 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.57 03:41:41.69 +41:30:55.2
153.97883 -10.87016 galactic Per Second-epoch detections are separated by 2.0" 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 | target | 03:41:41.69 +41:30:55.2 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 41 41.69 +41 30 55.2 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
target,2461119.5885,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:41.69 +41:30:55.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 47 34.56 +42 51 33.4 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
Gaia DR3 243260148716707968,2461119.5885,13.54,0.05,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 243260148716707968 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:34.56 +42:51:33.4 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 57.87 +41 37 04.9 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 237183727766572288,2461119.5885,13.54,0.05,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 237183727766572288 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:57.87 +41:37:04.9 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.57 03:42:31.75 +40:29:17.6
154.74935 -11.58329 galactic Per Second-epoch detections are separated by 1.3" 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 J055.6416+40.4902 | 03:42:31.75 +40:29:17.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A9V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 31.75 +40 29 17.6 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
ATO J055.6416+40.4902,2461119.5885,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J055.6416+40.4902 20260320.0885 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:31.75 +40:29:17.6 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.42 03:42:41.98 +40:21:49.2
154.85391 -11.66125 galactic Per Second-epoch detections are separated by 2.7" 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 224959494927620736 | 03:42:42.66 +40:21:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 41.98 +40 21 49.2 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 224959494927620736,2461119.5885,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 224959494927620736 20260320.0885 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:41.98 +40:21:49.2 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.39 03:43:36.35 +42:18:29.1
153.76822 -10.02639 galactic Per Second-epoch detections are separated by 4.3" 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 237264335713532928 | 03:43:35.23 +42:18:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 36.35 +42 18 29.1 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
Gaia DR3 237264335713532928,2461119.5885,13.39,0.05,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 237264335713532928 20260320.0885 13.39CV 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:36.35 +42:18:29.1 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.63 03:44:42.66 +42:16:54.9
153.94772 -9.92058 galactic Per Second-epoch detections are separated by 4.3" 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 243219020110319872 | 03:44:43.36 +42:16:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 44 42.66 +42 16 54.9 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
Gaia DR3 243219020110319872,2461119.5885,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 243219020110319872 20260320.0885 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:42.66 +42:16:54.9 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.65 03:46:09.03 +41:09:42.2
154.87015 -10.62995 galactic Per Second-epoch detections are separated by 0.8" 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 | target | 03:46:09.03 +41:09:42.2 (user input) | T | P | (position from user input) 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 03 20.0885* 03 46 09.03 +41 09 42.2 13.7 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
target,2461119.5885,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:09.03 +41:09:42.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.36 03:41:55.30 +42:04:28.5
153.66409 -10.40234 galactic Per Second-epoch detections are separated by 5.4" 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 237266367236365440 | 03:41:54.01 +42:04:30.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 41 55.30 +42 04 28.5 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 237266367236365440,2461119.5885,13.36,0.05,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 237266367236365440 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:55.30 +42:04:28.5 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.48 03:42:16.48 +40:00:27.1
155.01331 -11.99153 galactic Per Second-epoch detections are separated by 3.2" 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 | target | 03:42:16.48 +40:00:27.1 (user input) | T | P | (position from user input) 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 03 20.0885* 03 42 16.48 +40 00 27.1 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
target,2461119.5885,13.48,0.05,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
target 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:16.48 +40:00:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.38 03:47:36.35 +42:26:39.5
154.26910 -9.46020 galactic Per Second-epoch detections are separated by 1.9" 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 243238639520688512 | 03:47:37.07 +42:26:39.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 47 36.35 +42 26 39.5 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 243238639520688512,2461119.5885,13.38,0.05,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
Gaia DR3 243238639520688512 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:36.35 +42:26:39.5 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.48 03:43:27.46 +41:11:18.2
154.44929 -10.92415 galactic Per Second-epoch detections are separated by 2.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J055.8671+41.1886 | 03:43:27.46 +41:11:18.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 27.46 +41 11 18.2 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 J055.8671+41.1886,2461119.5885,13.48,0.05,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 J055.8671+41.1886 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:27.46 +41:11:18.2 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.61 03:42:12.25 +39:31:12.8
155.31024 -12.38320 galactic Per Second-epoch detections are separated by 4.0" 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 | target | 03:42:12.25 +39:31:12.8 (user input) | T | P | (position from user input) 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 03 20.0885* 03 42 12.25 +39 31 12.8 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
target,2461119.5885,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0885 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:12.25 +39:31:12.8 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.45 03:40:42.65 +42:31:34.8
153.20349 -10.18137 galactic Per Second-epoch detections are separated by 6.4" and 2.7 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 | target | 03:40:42.65 +42:31:34.8 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 40 42.65 +42 31 34.8 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
target,2461119.5885,13.45,0.05,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
target 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:42.65 +42:31:34.8 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.44 03:44:00.25 +41:43:08.6
154.19715 -10.44383 galactic Per Second-epoch detections are separated by 0.8" 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 J055.9947+41.7226 | 03:43:59.24 +41:43:09.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 03 20.0885* 03 44 00.25 +41 43 08.6 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 J055.9947+41.7226,2461119.5885,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J055.9947+41.7226 20260320.0885 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:00.25 +41:43:08.6 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 03.24 +40 37 42.2 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 225024610930731392,2461119.5885,13.27,0.05,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
Gaia DR3 225024610930731392 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:03.24 +40:37:42.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.21 03:41:19.62 +42:31:52.4
153.29188 -10.10829 galactic Per Second-epoch detections are separated by 3.0" and 2.7 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 J055.3432+42.5289 | 03:41:18.33 +42:31:54.2 (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 03 20.0885* 03 41 19.62 +42 31 52.4 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 J055.3432+42.5289,2461119.5885,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J055.3432+42.5289 20260320.0885 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:19.62 +42:31:52.4 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.23 03:44:19.70 +41:56:27.7
154.10567 -10.23213 galactic Per Second-epoch detections are separated by 8.2" 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 | ATO J056.0915+41.9425 | 03:44:19.70 +41:56:27.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 44 19.70 +41 56 27.7 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 J056.0915+41.9425,2461119.5885,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J056.0915+41.9425 20260320.0885 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:19.70 +41:56:27.7 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.29 03:43:14.43 +39:40:13.2
155.37559 -12.14172 galactic Per Second-epoch detections are separated by 2.7" 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 | Gaia DR3 224719908770603904 | 03:43:13.83 +39:40:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 14.43 +39 40 13.2 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 224719908770603904,2461119.5885,13.29,0.05,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 224719908770603904 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:14.43 +39:40:13.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.12 03:41:45.24 +40:09:32.4
154.83771 -11.93362 galactic Per Second-epoch detections are separated by 0.5" 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 | Gaia DR3 224980149429516032 | 03:41:45.84 +40:09:35.4 (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 03 20.0885* 03 41 45.24 +40 09 32.4 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
Gaia DR3 224980149429516032,2461119.5885,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 224980149429516032 20260320.0885 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:45.24 +40:09:32.4 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.15 03:44:12.57 +41:12:06.0
154.55401 -10.82614 galactic Per Second-epoch detections are separated by 1.5" 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 225138891420455680 | 03:44:13.31 +41:12:06.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 44 12.57 +41 12 06.0 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
Gaia DR3 225138891420455680,2461119.5885,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 225138891420455680 20260320.0885 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:12.57 +41:12:06.0 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.14 03:43:28.85 +42:09:00.2
153.84873 -10.16505 galactic Per Second-epoch detections are separated by 1.2" 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 J055.8568+42.1508 | 03:43:27.62 +42:09:02.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 28.85 +42 09 00.2 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 J055.8568+42.1508,2461119.5885,13.14,0.05,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
ATO J055.8568+42.1508 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:28.85 +42:09:00.2 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 13.06 03:43:04.75 +40:19:37.2
154.93509 -11.64537 galactic Per Second-epoch detections are separated by 1.7" 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 J055.7670+40.3267 | 03:43:04.08 +40:19:36.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 04.75 +40 19 37.2 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 J055.7670+40.3267,2461119.5885,13.06,0.05,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
ATO J055.7670+40.3267 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:04.75 +40:19:37.2 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 12.79 03:42:04.33 +42:44:25.3
153.27221 -9.85900 galactic Per Second-epoch detections are separated by 8.8" and 2.2 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 J055.5079+42.7378 | 03:42:03.51 +42:44:27.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 04.33 +42 44 25.3 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
ATO J055.5079+42.7378,2461119.5885,12.79,0.05,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
ATO J055.5079+42.7378 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:04.33 +42:44:25.3 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 12.88 03:43:44.89 +41:26:42.1
154.33136 -10.68873 galactic Per Second-epoch detections are separated by 0.2" 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 J055.9484+41.4462 | 03:43:45.60 +41:26:41.3 (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 03 20.0885* 03 43 44.89 +41 26 42.1 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 J055.9484+41.4462,2461119.5885,12.88,0.05,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 J055.9484+41.4462 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:44.89 +41:26:42.1 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 12.85 03:43:14.71 +40:30:26.0
154.84660 -11.48424 galactic Per Second-epoch detections are separated by 0.3" 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 | Gaia DR3 224966646052105728 | 03:43:15.31 +40:30:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 43 14.71 +40 30 26.0 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 224966646052105728,2461119.5885,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 224966646052105728 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:14.71 +40:30:26.0 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 12.79 03:41:51.24 +40:38:29.1
154.54993 -11.54158 galactic Per Second-epoch detections are separated by 1.0" 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 | Gaia DR3 225025538643358464 | 03:41:52.09 +40:38:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 41 51.24 +40 38 29.1 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 225025538643358464,2461119.5885,12.79,0.05,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
Gaia DR3 225025538643358464 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:51.24 +40:38:29.1 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 12.85 03:42:24.08 +39:37:28.0
155.27489 -12.27778 galactic Per Second-epoch detections are separated by 1.4" 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 | Gaia DR3 224901843585961728 | 03:42:23.24 +39:37:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 24.08 +39 37 28.0 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 224901843585961728,2461119.5885,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 224901843585961728 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:24.08 +39:37:28.0 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 12.62 03:43:26.39 +41:59:31.5
153.94166 -10.29408 galactic Per Second-epoch detections are separated by 0.9" 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 237209085254246784 | 03:43:26.97 +41:59:33.7 (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 03 20.0885* 03 43 26.39 +41 59 31.5 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 237209085254246784,2461119.5885,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 237209085254246784 20260320.0885 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:26.39 +41:59:31.5 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 42 27.96 +40 24 22.1 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 225007499781116288,2461119.5885,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 225007499781116288 20260320.0885 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:27.96 +40:24:22.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 12.44 03:46:35.83 +41:42:42.3
154.58677 -10.14844 galactic Per Second-epoch detections are separated by 0.8" 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 231168681907412224 | 03:46:36.54 +41:42:42.8 (Gaia DR3) | T | P | 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 03 20.0885* 03 46 35.83 +41 42 42.3 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 231168681907412224,2461119.5885,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 231168681907412224 20260320.0885 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:35.83 +41:42:42.3 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 10.45 03:41:22.32 +41:08:27.3
154.16383 -11.20316 galactic Per Second-epoch detections are separated by 0.3" 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 | Gaia DR3 237054436370621312 | 03:41:23.17 +41:08:29.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1949AnHar.112....1C HD 275596
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 41 22.32 +41 08 27.3 10.4 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 237054436370621312,2461119.5885,10.45,0.05,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
Gaia DR3 237054436370621312 20260320.0885 10.45CV 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:22.32 +41:08:27.3 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0885 2461119.5885 12.67 03:45:32.07 +34:51:31.7
158.85500 -15.59896 galactic Per Second-epoch detections are separated by 0.5" 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 | Gaia DR3 218337827886678528 | 03:45:31.96 +34:51:32.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 45 32.07 +34 51 31.7 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
Gaia DR3 218337827886678528,2461119.5885,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 218337827886678528 20260320.0885 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:32.07 +34:51:31.7 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 03 55 21.98 +41 12 48.2 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 J0355214+411242,2461119.5885,12.79,0.05,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 J0355214+411242 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:21.98 +41:12:48.2 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201972353223841152,2461119.5885,13.18,0.05,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 201972353223841152 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:32.61 +42:12:26.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 04 16 01.32 +37 20 29.1 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
NSVS J0416015+372028,2461119.5885,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0416015+372028 20260320.0885 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:01.32 +37:20:29.1 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 04 29 17.92 +42 33 35.4 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
GW Per,2461119.5885,12.02,0.05,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
GW Per 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:17.92 +42:33:35.4 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 04 19 09.15 +40 45 43.7 11.6 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
GL Per,2461119.5885,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GL Per 20260320.0885 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:19:09.15 +40:45:43.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 04 16 24.28 +39 25 45.6 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 J0416241+392545,2461119.5885,12.90,0.05,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
NSVS J0416241+392545 20260320.0885 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:24.28 +39:25:45.6 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 04 50 00.77 +39 55 57.8 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0450006+395559,2461119.5885,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0450006+395559 20260320.0885 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:00.77 +39:55:57.8 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0885* 04 44 41.94 +41 22 54.0 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
NSVS 4345711,2461119.5885,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 4345711 20260320.0885 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:44:41.94 +41:22:54.0 ;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-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20_00sec_-14_90C_LIGHT_0018_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: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
First image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Last image: 2461119.58871432 20.03.2026 02:07:34.917 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 25
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 18144
Objects passed selection criteria: 18134
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 17259.2
Average stars matched: 16864.8 (97.7143 %)
Memory usage VmPeak: 122552 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 21:34:09 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
First image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Last image: 2461119.58871432 20.03.2026 02:07:34.917 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 996
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 71 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): 129641
Objects passed selection criteria: 129401
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 119302
Average stars matched: 115361 (96.6964 %)
Memory usage VmPeak: 1955024 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 21:36:55 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
SExtractor catalog cache: saved Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461119.58819169
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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits exists and is non-empty
Saving wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits to local_wcs_cache/
'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'local_wcs_cache/wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits exists and is non-empty
Saving wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits to local_wcs_cache/
'wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits' -> 'local_wcs_cache/wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits'
wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.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 04:21:49.016 +37:59:51.53
Second-epoch image center 04:21:47.612 +37:59:47.93
Angular distance between the image centers 0.00 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 04:21:49.016 +37:59:51.53
Second-epoch image center 04:21:46.112 +37:59:57.73
Angular distance between the image centers 0.01 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 04:21:47.612 +37:59:47.93
Second-epoch second image center 04:21:46.112 +37:59:57.73
Angular distance between the image centers 0.00563 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits &> /tmp/tmp.lH1jOf8sTH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits &> /tmp/tmp.j4VCmhviqj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.g3VYx6eOkN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.h3lsZcqX7m
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
Found non-empty wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
The reference image (wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits) and catalog (wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat) found
'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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 7129 out of 18677 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.971832
a=0.000000 b=1.000000 c=22.971832
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 22 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
2.1 pix Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
2.6 pix fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
2.6 pix fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.4 mag. Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
15.4 mag. Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
15.1 mag. fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
15.1 mag. fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.3 (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.lH1jOf8sTH (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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1808, passed=18677
Got 18677 stars (including 16842 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
util/solve_plate_with_UCAC5 got 18677 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 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 961 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: 0.37"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -region wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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.j4VCmhviqj (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-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits' -> 'wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1789, passed=18684
Got 18684 stars (including 16861 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat
util/solve_plate_with_UCAC5 got 18684 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 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 961 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: 0.37"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits -region wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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.g3VYx6eOkN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1205, passed=16024
Got 16024 stars (including 14802 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 16024 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 962 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: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.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.h3lsZcqX7m (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1190, passed=16166
Got 16166 stars (including 14962 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 16166 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 962 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
Saving fully-calibrated image wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits'
Preparing the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out08898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21230.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21201_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21201_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:47:16.86 +33:19:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.967 161455311079612800 071.82055068641 +33.32282168301 12.1374 11.3853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21202_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 21202_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21208_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 21208_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21215_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 21215_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21230_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 21230_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21244_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21244_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:02:38.07 +32:55:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 0.261 170247972427945344 060.65864326890 +32.91795680146 11.1920 10.4012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21245_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21245_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:57:40.37 +41:54:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 1.844 201869033488805504 074.41883762352 +41.91287603518 11.6962 10.8637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21247_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21247_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:19:09.12 +40:45:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.156 227882791407954432 064.78758110444 +40.76206204066 10.8387 9.4385 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21256_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21256_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:52:41.66 +42:36:21.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21268_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21268_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:29:17.92 +42:33:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.730 252291361131508864 067.32481178178 +42.56035745697 12.8345 10.7906 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21284_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21284_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:20:52.49 +41:03:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 1.356 227904678561057536 065.21829325497 +41.05829269826 10.4364 8.9041 VARIABLE#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 21291_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21291_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:26:02.06 +39:13:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.392 179478059005516416 066.50850920635 +39.22571299907 12.0839 11.5028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21294_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21294_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:56:16.15 +41:59:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 5.360 231377486037723776 059.06540884932 +41.99125808490 11.1711 9.8082 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21299_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21299_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:01:43.15 +40:43:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.746 200813536686643712 075.43042568241 +40.72332376130 11.9194 11.0418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21305_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21305_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:35:11.45 +40:23:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.394 203792659142334208 068.79783603968 +40.38611656855 11.9784 11.1380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21311_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21311_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:22:03.02 +40:03:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.027 227602141065072000 065.51285648083 +40.05255516216 12.4412 11.9256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21315_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21315_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:10:13.79 +39:05:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.672 226156626870904192 062.55744649530 +39.09634141579 11.8160 10.7182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21327_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21327_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:19:34.41 +38:31:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.280 179387658533875968 064.89342015393 +38.52806953329 12.3392 11.7116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21329_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21329_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:46:23.86 +39:15:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.290 199738587973233536 071.59948778821 +39.26005236923 12.1691 11.4551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21332_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 21332_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:59:17.60 +41:36:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.011 201752412239536256 074.82405882804 +41.60168881068 12.1836 11.3680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08898_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 08898_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14344_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 14344_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 21s
Prepared the HTML report for the field Per-05-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 ####
04:29:15.07 +39:33:44.0
04:15:40.68 +35:31:59.3
03:42:34.79 +41:05:34.3
03:41:34.73 +41:05:57.2
03:47:51.39 +42:24:54.6
03:51:17.02 +33:02:15.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
SExtractor catalog cache: saved Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Creating symlink local_wcs_cache/wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits exists and is non-empty
wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits exists and is non-empty
wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.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 04:21:49.016 +37:59:51.53
Second-epoch image center 04:21:47.612 +37:59:47.93
Angular distance between the image centers 0.00 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 04:21:49.016 +37:59:51.53
Second-epoch image center 04:21:46.112 +37:59:57.73
Angular distance between the image centers 0.01 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 04:21:47.612 +37:59:47.93
Second-epoch second image center 04:21:46.112 +37:59:57.73
Angular distance between the image centers 0.00563 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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits &> /tmp/tmp.DUvJY9MG7Z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits &> /tmp/tmp.WZpC2krro0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.sHNGzdS0mY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.rjUH1ckSkU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
Found non-empty wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
The reference image (wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits) and catalog (wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat) found
'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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 7196 out of 137281 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.837428
a=0.000000 b=1.000000 c=22.837428
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.54
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 569 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
2.0 pix Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
2.4 pix fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
2.4 pix fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.5 mag. Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
15.5 mag. Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
15.2 mag. fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
15.2 mag. fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.DUvJY9MG7Z (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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=15371, passed=137258
Got 137258 stars (including 121598 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
util/solve_plate_with_UCAC5 got 137258 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -region wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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.WZpC2krro0 (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-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits' -> 'wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS_IMAGE_NAME=wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS-calibrated image found: wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Checking if the catalog wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS catalog name: wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=15060, passed=136498
Got 136498 stars (including 121185 good ones) from the SExtractor catalog wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat
util/solve_plate_with_UCAC5 got 136498 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 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-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits -region wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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.sHNGzdS0mY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=10340, passed=103730
Got 103730 stars (including 93250 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 103730 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 958 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: 0.63"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.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.rjUH1ckSkU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=10481, passed=103820
Got 103820 stars (including 93181 good ones) from the SExtractor catalog wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 103820 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 957 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: 0.62"
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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/wcs_Per-05-Q2b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Saving fully-calibrated image wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/wcs_Per-05-Q2b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/wcs_fd_Per-05-Q2b1x1_2026-03-19_21-06-49_20.00sec_-14.90C_LIGHT_0018.fits
Saving fully-calibrated image wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Per-05-Q2b1x1_213145_TTUQ2b1x1_18323_mJpAMLhz/wcs_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019.fits
Preparing the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out07097.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out10702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out147906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159689.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160689.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160808.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out159617.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out08222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87160.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 116s
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: 40s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159326_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159326_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:51:40.31 +32:46:04.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159330_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159330_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:02.82 +34:23:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.749 218285944681874944 056.26199070783 +34.38497882879 13.6138 13.0661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159345_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159345_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:22:49.18 +35:36:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.163 176528138027772672 065.70495128577 +35.61427022495 14.3467 13.5358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159347_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159347_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:53:09.94 +33:38:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.208 161627766903867392 073.29144189634 +33.63358166659 13.9676 12.9496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159348_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159348_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159352_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159352_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:10:02.17 +39:04:49.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159360_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159360_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159363_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159363_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:47.01 +40:38:12.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159366_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159366_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:49:30.60 +34:00:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.981 218040066394767488 057.37687703628 +34.00119857785 13.8985 13.1611 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159368_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159368_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:48:20.30 +41:21:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 2.899 231101371180267264 057.08375533407 +41.35742866390 13.6513 12.9583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159371_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159371_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:53:49.83 +39:29:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.059 199909119651782400 073.45799555048 +39.49554148747 14.0876 13.1771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159375_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159375_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:46:19.60 +40:22:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.579 224856488730370816 056.58104252354 +40.37335320433 13.5355 12.9771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159380_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159380_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:24.17 +35:15:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 2.063 218402733432125696 056.35120509878 +35.26373823249 13.7527 13.1091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159389_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159389_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159392_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159392_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:02:12.34 +41:38:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 5.290 201717403965556224 075.55252684075 +41.63732382553 13.9764 13.1562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159399_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159399_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:02:51.12 +40:04:35.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159400_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159400_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:08.82 +40:17:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.573 224950222097226880 056.03670474555 +40.29551661823 13.6315 12.8695 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159401_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159401_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:59:12.51 +38:40:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 0.619 198952750695159040 074.80224398398 +38.67166095361 14.1766 13.5918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159406_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159406_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:36:01.35 +40:19:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.558 203039463615053824 069.00526803201 +40.31724669247 14.3844 13.8966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159409_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159409_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:44.81 +39:35:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.365 224713582281845120 055.68755810118 +39.59185779180 13.2745 12.4617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159411_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159411_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:00:07.95 +42:02:57.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159416_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159416_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:12.16 +39:07:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 4.208 224327176961144192 055.55201212960 +39.12963719778 13.1065 12.3979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159419_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159419_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:52:55.60 +33:56:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 0.912 161687479833305856 073.23193810825 +33.93386599438 14.2459 13.3318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159420_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159420_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159421_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159421_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:52.78 +42:40:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 4.638 243289526292868224 055.96820565812 +42.68297123168 13.2501 12.6438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159423_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159423_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:46:25.50 +42:42:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.886 243255063475552896 056.60568861570 +42.70898977749 13.4106 12.7635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159424_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159424_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159425_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159425_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:24.77 +40:07:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 4.898 224941494723796864 055.85400451868 +40.12039442282 13.4330 12.8667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159426_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159426_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:24.16 +42:08:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.864 243213591271743360 056.10127851525 +42.14386148160 13.4421 12.9369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159429_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159429_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:48:08.32 +42:35:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 3.205 243241044702278400 057.03586087752 +42.58744375096 13.3901 12.8042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159432_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159432_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:20.17 +40:33:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.451 225011726028545664 055.58326300517 +40.56191236907 13.2822 12.6593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159433_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159433_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:51.95 +41:31:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 3.949 225172735762659712 056.21792229085 +41.53257895228 13.0586 12.3062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159434_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159434_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:55:55.20 +41:53:53.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159435_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159435_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159437_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159437_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:21:51.21 +33:46:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.426 175788411517783040 065.46347035714 +33.76913429752 13.5906 12.5925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159439_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159439_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:49.77 +38:11:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 4.294 224204856293167232 055.70586263060 +38.19526707399 13.3884 12.7863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159441_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159441_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:46:15.04 +41:07:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 3.132 225102332659069696 056.56368760152 +41.12789845006 13.4025 12.7839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159444_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159444_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159452_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159452_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159454_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159454_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:30.23 +36:51:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.691 223058477980628096 056.12651784467 +36.85198732450 13.5253 12.9500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159461_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159461_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159462_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159462_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:53:26.18 +42:46:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.762 231295709860441344 058.35974241680 +42.77193566634 13.3489 12.6551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159467_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159467_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159468_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159468_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:55:23.30 +34:33:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.260 218869338680402176 058.84680420356 +34.56293062797 13.7651 12.9159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159471_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159471_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:16:45.89 +40:47:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.580 227929932968664320 064.19135667520 +40.79454792950 13.7693 12.8405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159473_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159473_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159474_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159474_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:01.70 +42:28:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 3.392 243274098770811776 056.25835655407 +42.46701797393 13.0722 12.3353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159477_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159477_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:54:18.89 +33:35:28.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159479_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159479_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:48:20.67 +42:00:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.390 231199227714643328 057.08570810438 +42.00254739262 13.1082 12.4411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159482_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159482_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:59:39.58 +33:08:04.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159483_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159483_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:12.13 +41:08:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.521 225140471968460032 055.80041797014 +41.13616639232 12.9733 12.1980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159488_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159488_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:17.55 +39:35:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.294 224900331757482496 055.57249615995 +39.59850263074 13.2606 12.7175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159489_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159489_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:41:30.60 +40:54:42.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159493_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159493_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:45.55 +41:08:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 3.176 225100408513731456 056.44084480052 +41.14894182154 13.2164 12.5936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159496_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159496_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:10.50 +40:17:47.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159497_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159497_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:28.84 +36:08:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.575 222953027943740672 056.12036038340 +36.13766254715 13.2604 12.3643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159498_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159498_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:50:58.60 +42:43:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.007 231318421647249792 057.74421831178 +42.72205625240 13.2604 12.6451 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159500_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159500_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159502_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159502_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:02.82 +39:57:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.783 224914934646129664 055.76074564146 +39.95459684688 13.1413 12.4109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159503_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159503_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159504_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159504_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:02:09.30 +41:46:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.705 201732346150761088 075.53855995268 +41.77582958582 13.8364 13.4579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159509_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159509_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159510_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159510_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:48:15.90 +42:42:45.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159511_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159511_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:47:50.84 +42:20:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.289 231221698983427328 056.96305921457 +42.33828394265 13.0324 12.2374 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159512_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159512_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:44.71 +41:55:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 4.622 237203523275372160 055.68457814169 +41.92993001496 13.0026 12.2241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159514_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159514_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159515_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159515_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159516_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159516_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159518_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159518_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159519_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159519_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:35.07 +39:03:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 3.216 224265157633358976 055.89514414529 +39.05538359139 13.3460 12.7822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159520_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159520_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:46:48.53 +34:28:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 0.875 218103425752035328 056.70191627527 +34.48308840762 13.5251 12.5702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159523_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159523_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:25.61 +40:13:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 4.174 224850956809651200 056.35765652429 +40.22218330077 13.1143 12.3489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159527_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159527_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:44:15.21 +35:05:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.234 174235553204545280 071.06374489694 +35.09339488991 13.3821 12.4167 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159528_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159528_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159534_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159534_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159540_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159540_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:31.73 +42:20:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.575 243222456084087168 056.38211611364 +42.33988001656 12.7360 11.8571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159544_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159544_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159545_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159545_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:41:32.79 +40:36:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.855 225025229405735040 055.38599097670 +40.61145505969 13.0995 12.5368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159546_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159546_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:58:16.33 +42:22:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.997 202031245815429248 074.56895367698 +42.37737204493 13.5301 12.4600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159549_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159549_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159554_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159554_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:02:12.65 +42:15:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 3.341 201797565234283136 075.55240709048 +42.26004360179 13.8697 13.2990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159555_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159555_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159556_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159556_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:20.16 +39:54:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.935 224747220465545216 056.08499565005 +39.91059114658 13.0840 12.5027 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159560_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159560_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159561_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159561_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:08.62 +40:15:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.204 224947954354512768 056.03404423786 +40.25950301342 12.9462 12.1375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159562_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159562_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:47:12.23 +42:47:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.648 243261042069954688 056.80266559085 +42.79052101822 12.9136 12.2896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159564_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159564_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159566_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159566_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:58.14 +41:54:10.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159572_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159572_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:39.23 +42:36:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 3.462 237471185637606912 055.66219947474 +42.61340868429 13.0823 12.5898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159576_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159576_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159577_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159577_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159578_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159578_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159583_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159583_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:47:39.26 +42:02:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.474 231202663688490880 056.91167914911 +42.04516349353 12.8661 12.2751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159587_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159587_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:10:51.73 +37:40:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.632 225443284344783232 062.71496977916 +37.66913487794 13.5288 12.6467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159589_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159589_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:30.30 +40:30:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.035 225057493200828160 056.12761965276 +40.50971991090 12.9583 12.3757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159590_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159590_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:56.39 +41:03:54.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159592_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159592_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159594_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159594_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:41:10.54 +42:38:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 3.117 237480806363820416 055.29497649986 +42.63493210040 12.7349 12.1359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159596_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159596_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:47:03.26 +40:55:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.920 225084499955252608 056.76391192691 +40.91888384467 12.9084 12.3021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159597_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159597_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159598_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159598_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159599_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159599_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159604_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159604_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159606_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159606_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:04:53.92 +34:07:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.892 170888884627655424 061.22448447138 +34.12180332188 13.4967 12.7860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159612_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159612_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:10.07 +39:28:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.530 224675825226274304 056.29152111133 +39.47882518178 12.9454 12.3435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159613_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159613_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159614_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159614_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159615_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159615_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:46:41.37 +41:58:37.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159616_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159616_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159617_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159617_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:52.26 +41:17:11.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159618_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159618_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159623_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159623_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159625_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159625_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159626_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159626_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159628_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159628_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:08.45 +42:17:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 5.580 237264752328985088 055.78311336147 +42.28411558973 12.7534 12.2156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159629_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159629_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159642_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159642_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:12.00 +40:57:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 5.308 225129717370395136 055.80194341178 +40.95991471764 12.7407 12.2302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159644_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159644_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:04.69 +42:29:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.602 237278977260104704 055.76901487160 +42.49799481974 12.8348 12.2716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159646_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159646_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159647_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159647_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159648_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159648_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159649_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159649_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:44.63 +35:57:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.117 221448896037014528 055.93661768361 +35.95508015093 12.9840 12.4522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159653_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159653_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159654_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159654_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:42.75 +41:37:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.223 231178921109518208 056.42618980458 +41.62772161157 12.8095 12.1970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159655_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159655_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159657_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159657_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:37.29 +42:27:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.139 237281549941810816 055.65495731127 +42.45632122951 12.6709 12.0864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159659_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159659_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159660_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159660_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:54:01.71 +33:23:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 4.389 218513681027620096 058.50856931520 +33.39973744444 13.7596 13.3401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159661_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159661_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159662_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159662_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159663_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159663_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:54.50 +34:30:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.304 218291785837372672 056.22709510555 +34.50311012200 13.0502 12.1892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159667_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159667_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:45.22 +40:57:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 5.746 225118035059665024 055.94048997129 +40.96391230950 12.7385 12.1657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159669_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159669_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159673_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159673_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159674_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159674_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:09.16 +41:29:26.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159675_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159675_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159682_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159682_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:15.68 +42:32:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 5.220 243283925655564288 055.81729154164 +42.53956141478 12.1724 11.4146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159683_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159683_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159684_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159684_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159686_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159686_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:57.73 +41:52:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 5.550 237193009195402368 055.98850911620 +41.86826298693 12.6050 11.9244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159687_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159687_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159689_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159689_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:47:33.25 +42:03:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.521 231202904206659712 056.89022777012 +42.05337681650 12.5862 12.0377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159692_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159692_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:41:48.60 +40:05:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.025 224931255521851264 055.45131720714 +40.08529526518 12.7434 12.2905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159699_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159699_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:56:08.51 +35:17:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.346 218960976102078976 059.03508464010 +35.28793867359 13.1407 12.3812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159700_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159700_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159703_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159703_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159705_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159705_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159710_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159710_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:59.02 +39:36:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.859 224713483500069888 055.74730730502 +39.61225637498 12.6016 12.0034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159711_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159711_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159712_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159712_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159716_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159716_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:46:55.99 +41:56:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.948 231189946286453632 056.73433428176 +41.93609869818 12.4019 11.6001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159719_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159719_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:46:06.52 +42:34:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.190 243252001159866368 056.52761362892 +42.57926629528 12.3988 11.7718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159720_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159720_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:54.15 +41:28:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.501 225160744214186752 056.47445991783 +41.47551547680 12.4810 11.9306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159722_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159722_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159723_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159723_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159726_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159726_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:10.79 +40:00:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.874 224752275643926400 056.29511713140 +40.00325625509 12.5174 11.7804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159728_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159728_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:13.62 +39:42:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 4.649 224729765717415424 056.30836724964 +39.71679149872 12.4053 11.6724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159731_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159731_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:21.52 +42:19:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.047 243266951945340416 056.09144538316 +42.32245762090 12.3112 11.6071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159732_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159732_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159738_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159738_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159740_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159740_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159743_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159743_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159749_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159749_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:59:16.57 +33:05:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.271 170405580546662912 059.81901318356 +33.09570329573 12.9884 12.2530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159750_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159750_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:41:19.59 +41:07:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.899 237054024053767936 055.33096542765 +41.12593428055 12.1780 11.6180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159754_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159754_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159755_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159755_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159758_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159758_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:03:50.00 +35:00:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.175 219039208927401856 060.95814287468 +35.00876872048 12.7580 12.0087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159760_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159760_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:41.28 +41:54:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.797 237205138183036800 055.92027316946 +41.90965766299 12.0882 11.5445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159761_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159761_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:47:54.56 +42:08:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.254 231204690913007872 056.97892437637 +42.13407399133 12.1498 11.5786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159763_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159763_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:01:11.14 +40:55:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 0.489 200830991433512448 075.29638264953 +40.92569996108 12.6741 12.1903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159764_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159764_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159765_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159765_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:23.63 +42:26:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 5.003 237280763966520832 055.60033892293 +42.44971527317 12.0607 11.2974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159768_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159768_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:54.13 +35:48:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.437 221443913874979072 055.97675234278 +35.80766157517 12.0332 11.3448 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159770_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159770_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159777_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159777_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159778_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159778_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159779_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159779_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159782_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159782_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:18.46 +41:06:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 2.842 225125525482555136 056.07796399789 +41.10079402858 12.1360 11.5505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159783_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159783_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:02:09.00 +42:06:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.634 201792376913912192 075.53664316507 +42.10169351929 12.7202 12.4889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159785_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159785_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159788_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159788_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159793_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159793_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:44:38.21 +42:01:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 5.022 243200358473132544 056.16102756840 +42.03101266027 11.7721 11.2007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159795_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159795_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:00.84 +40:34:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.367 225047906833774080 056.25453380584 +40.57795250937 12.0877 11.7202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159798_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159798_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:10.77 +42:13:47.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159799_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159799_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:34.59 +41:05:34.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159803_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159803_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:32.06 +40:01:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.444 224928369303818752 055.63404670073 +40.03267395124 11.9303 11.3866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159804_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159804_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159805_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159805_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159807_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159807_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159809_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159809_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159811_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159811_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:02:10.63 +41:57:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 2.255 201743135108254080 075.54511257678 +41.95527947703 12.1228 11.3520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159812_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159812_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:38.03 +40:29:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 4.045 224967127088434048 055.90698095307 +40.48986325690 11.4695 10.8407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159817_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159817_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159820_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159820_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:01:58.40 +39:06:09.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159824_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159824_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:42:03.03 +42:13:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 5.197 237269562691932160 055.51444724771 +42.22759655042 10.4369 9.6692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159825_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159825_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159828_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159828_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159829_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 159829_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159858_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159858_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159859_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159859_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:02:38.09 +32:55:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 0.406 170247972427945344 060.65864326890 +32.91795680146 11.1920 10.4012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159860_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159860_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:57:40.40 +41:54:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 1.543 201869033488805504 074.41883762352 +41.91287603518 11.6962 10.8637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159868_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159868_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159870_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159870_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:52:41.67 +42:36:20.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159879_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159879_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159882_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159882_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159885_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159885_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159899_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159899_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159900_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159900_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159904_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159904_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159907_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159907_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159913_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159913_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:52:27.83 +39:15:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.818 199878741345621632 073.11591293965 +39.26635896190 12.3510 11.7562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159915_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159915_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159917_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159917_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159925_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159925_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159932_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159932_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159941_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159941_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159943_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159943_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159948_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159948_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159954_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159954_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159955_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159955_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159959_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159959_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159960_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159960_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159961_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159961_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159962_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159962_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159969_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159969_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159972_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159972_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159974_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159974_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159981_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159981_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159982_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159982_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159983_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159983_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159987_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159987_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159989_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159989_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159991_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159991_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159992_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159992_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:01:28.97 +40:30:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.776 200807214494940160 075.37099012431 +40.50927362678 12.6502 12.0917 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159995_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159995_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159999_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 159999_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:39:22.53 +40:31:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.478 203058597692894464 069.84404175917 +40.53228926803 12.3110 11.2846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160003_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160003_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160004_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160004_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:24:24.67 +41:42:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 0.631 228134167253355776 066.10281114361 +41.70740866950 12.7178 12.1030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160007_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160007_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:09:00.12 +41:28:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 0.541 228909765328338304 062.25056383885 +41.47913537045 12.6930 12.0993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160011_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160011_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160013_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160013_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160015_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160015_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160018_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160018_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160022_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160022_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160023_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160023_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160024_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160024_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160025_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160025_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160026_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160026_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160027_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160027_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160030_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160030_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160031_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160031_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160032_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160032_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:58:54.43 +41:03:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.532 201595594391694848 074.72732301371 +41.05200449046 12.7647 11.9271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160035_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160035_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160038_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160038_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160043_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160043_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160046_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160046_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160047_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160047_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160049_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160049_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160051_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160051_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:02:43.20 +41:05:35.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160052_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160052_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160060_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160060_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160061_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160061_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160064_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160064_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160065_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160065_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160066_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160066_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160068_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160068_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160069_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160069_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160077_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160077_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160079_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160079_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160081_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160081_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160087_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160087_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160091_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160091_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160092_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160092_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160093_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160093_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160095_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160095_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160096_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160096_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160098_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160098_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160100_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160100_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:00:17.36 +37:48:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.542 198765764998444160 075.07234627912 +37.81181698081 13.2373 12.5770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160103_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160103_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:51:45.71 +34:21:51.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160105_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160105_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160108_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160108_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160112_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160112_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:12:13.77 +36:19:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.730 177268865267438336 063.05754475691 +36.31723287072 13.3849 12.8408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160113_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160113_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160117_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160117_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:52:20.58 +35:29:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.863 219765062699879424 058.08600098492 +35.49193064386 13.1700 12.6275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160119_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160119_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160121_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160121_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160124_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160124_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160129_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160129_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:01:48.75 +42:09:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.907 201790830725676672 075.45496334179 +42.16518649006 13.2073 12.5879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160131_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160131_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:55:13.81 +36:20:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.368 220194044033008896 058.80746931081 +36.33963823483 13.2912 12.8511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160139_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160139_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160143_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160143_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160146_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160146_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:00:33.03 +42:14:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.976 230646482603107200 060.13830050449 +42.24082950203 13.3304 12.7562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160147_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160147_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160149_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160149_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160150_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160150_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160152_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160152_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160156_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160156_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160158_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160158_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160168_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160168_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160171_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160171_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160172_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160172_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160175_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160175_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160176_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160176_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160178_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160178_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160190_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160190_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160191_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160191_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:17:52.22 +42:00:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 0.776 228763495924548736 064.46786578726 +42.00547869231 12.2024 10.8547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160192_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160192_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160197_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160197_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:51:37.81 +42:24:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.555 203500536946333184 072.90738735276 +42.40624269862 13.4746 12.4129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160198_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160198_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160200_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160200_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160201_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160201_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:01:49.35 +41:11:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.216 200934689125035520 075.45629935011 +41.18767920141 13.2949 12.3502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160203_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160203_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160209_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160209_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160211_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160211_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160212_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160212_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160214_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160214_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160215_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160215_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160216_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160216_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:58.03 +38:23:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 5.403 223481583799147264 055.98995138400 +38.39891567962 13.1632 12.3000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160217_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160217_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:59:26.20 +37:53:18.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160218_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160218_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:01:50.02 +41:38:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 4.495 201717953721396736 075.45680745156 +41.63491419387 14.0722 13.7412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160219_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160219_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:13:21.32 +33:28:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.175 169928461222245760 063.33902158946 +33.48134182336 13.3840 12.5395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160221_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160221_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:02:22.67 +40:26:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.558 200759862476843520 075.59484197209 +40.44311991787 13.4453 12.5831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160222_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160222_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160223_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160223_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:52:20.66 +42:24:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.407 204989271394939392 073.08572136974 +42.40228519156 13.4497 12.8195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160224_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160224_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:00:32.70 +42:14:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.095 230646482603105536 060.13624303879 +42.24844260141 13.0323 12.0998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160228_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160228_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160230_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160230_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160231_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160231_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160234_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160234_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160235_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160235_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160239_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160239_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160240_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160240_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160241_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160241_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160244_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160244_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160247_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160247_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160250_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160250_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:50:35.30 +42:36:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.440 231316016465606912 057.64661121727 +42.61449866676 12.9064 11.9465 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160263_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160263_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:49:56.53 +41:49:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.755 203424185311967104 072.48563321589 +41.81783728517 13.5370 13.0355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160264_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160264_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:59:49.91 +41:52:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.059 201774196315797120 074.95758733181 +41.87845476207 13.4597 13.0455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160266_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160266_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160270_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160270_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:08:57.18 +42:14:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.139 231947995136526336 062.23751479926 +42.23665502168 13.0761 12.0996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160271_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160271_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:57:43.53 +42:37:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 5.148 202051616839618816 074.43251255695 +42.62709059140 13.6400 13.1352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160274_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160274_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160276_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160276_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160278_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160278_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:50:43.97 +42:20:38.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160279_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160279_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160280_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160280_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160284_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160284_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160290_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160290_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:07:38.69 +35:41:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.243 177141635457106816 061.91113292280 +35.69447143667 13.5912 12.9919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160291_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160291_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160293_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160293_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:03:08.98 +34:51:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.764 219030623292375680 060.78685119514 +34.85410163156 13.8453 13.2835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160299_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160299_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160303_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160303_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160307_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160307_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160310_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160310_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160312_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160312_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160313_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160313_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160315_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160315_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:19:39.89 +34:18:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.673 175876441167409024 064.91606656030 +34.31329861419 13.7402 13.0854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160320_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160320_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160322_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160322_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:54:52.02 +39:05:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.744 199130077005857536 073.71729653031 +39.09178968103 13.6017 12.5615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160323_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160323_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160327_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160327_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160331_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160331_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:33:09.35 +41:39:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.254 204099697765248896 068.28938553851 +41.65758421594 13.4152 12.4314 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160333_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160333_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:53:41.77 +38:47:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.368 199101077386695808 073.42442328644 +38.78887538492 13.5340 12.7580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160339_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160339_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160340_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160340_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160341_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160341_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160343_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160343_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160345_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160345_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160346_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160346_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:57:23.50 +35:19:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 2.016 218964274637187328 059.34852610610 +35.33202022875 13.9402 13.3391 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160347_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160347_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160348_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160348_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160355_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160355_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160356_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160356_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160357_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160357_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160367_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160367_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160369_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160369_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160371_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160371_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:27:10.65 +35:29:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.097 176372625852893568 066.79401268461 +35.49661817225 12.2474 10.8098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160372_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160372_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160374_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160374_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:57:01.10 +37:52:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.425 198805209977915008 074.25463978857 +37.88208164456 13.8348 13.2910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160376_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160376_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160381_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160381_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160384_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160384_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:10:46.22 +38:03:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.321 226026747060296576 062.69223926507 +38.05536379933 13.4348 12.4798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160388_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160388_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160389_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160389_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160390_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160390_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160394_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160394_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160399_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160399_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:57:22.60 +41:48:58.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160400_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160400_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:08:08.79 +37:44:40.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160409_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160409_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160415_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160415_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160416_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160416_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160418_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160418_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160419_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160419_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160420_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160420_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:13:10.85 +33:30:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 4.977 169928770459892736 063.29429564832 +33.50179019392 14.6133 13.9846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160421_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160421_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160424_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160424_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160425_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160425_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160427_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160427_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160432_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160432_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:49:55.13 +41:49:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.107 203424357111015168 072.47940480830 +41.82437495709 13.5706 12.4881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160433_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160433_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:57:26.06 +38:50:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.234 199055447653618048 074.35856811376 +38.84024160991 14.2312 13.6031 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160436_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160436_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160439_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160439_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160440_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160440_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160441_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160441_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:23:11.53 +35:29:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 3.950 176523327664406144 065.79911208903 +35.48802779733 13.6497 12.6408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160443_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160443_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160444_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160444_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160447_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160447_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160449_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160449_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160450_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160450_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160454_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160454_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160457_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160457_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160461_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160461_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160462_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160462_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160464_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160464_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:04:45.86 +42:16:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.872 230517564865783808 061.19141041946 +42.27201051452 13.7561 13.0365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160470_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160470_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160471_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160471_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160472_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160472_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160475_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160475_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:02:13.97 +41:24:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.135 201688507425692160 075.55786003558 +41.40102322157 13.9367 13.3387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160477_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160477_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160478_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160478_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160480_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160480_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:18:33.43 +33:48:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.963 175754154858113920 064.63974263910 +33.80689625212 14.2089 13.6029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160487_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160487_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:54:49.43 +40:39:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 4.496 200114865765313792 073.70705637839 +40.65504173633 14.1448 13.5494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160490_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160490_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160495_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160495_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:12:42.50 +39:23:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 4.152 226246786823603968 063.17684977944 +39.38955538564 14.4179 13.6590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160497_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160497_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:10:49.13 +42:10:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 3.458 228953367836334208 062.70392630863 +42.17631744529 13.6261 12.7272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160504_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160504_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160505_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160505_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:23:12.57 +35:29:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.298 176523435040661760 065.80281534036 +35.49593483788 13.9469 13.2287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160509_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160509_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:20:03.82 +40:30:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.387 227677114013806080 065.01588483188 +40.51313257246 14.0514 13.3521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160513_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160513_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:00:58.48 +40:30:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.604 200804259557492480 075.24335828910 +40.50560122794 14.0429 13.5835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160514_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160514_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:49:57.23 +42:36:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 2.387 203702842790275840 072.48933199723 +42.60616210512 13.7313 12.6524 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160515_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160515_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160516_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160516_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160517_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160517_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:55:59.69 +40:10:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.619 200042504156774272 073.99842578643 +40.16993874180 14.2560 13.7618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160519_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160519_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:03:06.98 +41:37:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 3.400 200970212795371392 075.77990079327 +41.62630775283 14.0637 13.5870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160524_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160524_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:54:59.45 +40:45:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.508 200124520851753344 073.74760091701 +40.76269195513 14.5193 13.7268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160527_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160527_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160528_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160528_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160531_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160531_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160532_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160532_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:32:53.39 +32:52:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.738 172087592817563648 068.22230636376 +32.86920054709 13.7167 12.8539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160539_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160539_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:08:23.64 +41:28:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.826 227412544029133312 062.09904017263 +41.47436095935 13.8934 13.1555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160541_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160541_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160543_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160543_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160545_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160545_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:50:16.75 +38:45:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 3.434 199485631578570880 072.57048630197 +38.76534085320 14.0578 13.4203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160546_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160546_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:49:35.05 +39:13:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 3.220 199558989619949952 072.39700209778 +39.21883700191 14.0324 13.3773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160548_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160548_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160551_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160551_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160558_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160558_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160560_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160560_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160564_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160564_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160565_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160565_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160568_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160568_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:26:37.20 +43:01:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 3.443 228537206987032704 066.65420744606 +43.02112188284 14.0747 13.4329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160570_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160570_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:11:27.76 +36:49:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.396 225333504981330176 062.86574031555 +36.82557379263 14.1622 13.4655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160571_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160571_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:02:12.68 +41:25:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.636 201688816663326848 075.55252780609 +41.42572566883 14.1785 13.8040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160573_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160573_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:18:16.47 +34:47:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 3.520 176094934743478656 064.56872877167 +34.79005378460 14.2645 13.4672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160577_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160577_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160578_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160578_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:24:27.20 +42:45:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 5.382 228515727848508672 066.11313827379 +42.76298396862 14.2491 13.5490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160584_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160584_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160585_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160585_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160586_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160586_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160587_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160587_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:08:14.37 +41:28:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 4.016 227412440949277824 062.05839263149 +41.48189524938 13.9082 13.1006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160588_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160588_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160590_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160590_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160592_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160592_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:01:20.01 +39:34:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.807 226814925097934464 060.33346817960 +39.57591993462 13.8185 12.7934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160594_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160594_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:14:07.87 +35:48:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 2.126 177008491468799232 063.53310730217 +35.81588452982 14.3490 13.7168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160596_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160596_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160599_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160599_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160603_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160603_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:54:11.99 +41:01:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 4.153 200319168770217856 073.54879893299 +41.02841896349 14.3365 13.7091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160606_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160606_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160608_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160608_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160614_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160614_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160619_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160619_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:29:15.12 +39:20:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 4.108 179661475586663680 067.31372998746 +39.34310270886 15.2024 13.8900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160620_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160620_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160621_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160621_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160622_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160622_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160623_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160623_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160624_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160624_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:11:08.11 +40:08:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 2.791 227063376068008192 062.78278483879 +40.14917774138 12.0847 10.3159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160634_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160634_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160637_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160637_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160640_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160640_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160642_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160642_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160643_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160643_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:03:07.40 +34:31:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 0.371 170960215444202368 060.78093711645 +34.52450185263 14.2488 13.4915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160646_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160646_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160650_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160650_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160653_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160653_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160654_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160654_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160664_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160664_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160667_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160667_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160668_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160668_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160670_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160670_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:56:01.86 +40:00:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.812 200005464358875392 074.00812594850 +40.00494061687 14.0396 13.0754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160671_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160671_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:41:43.88 +40:30:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 3.469 203094164319562368 070.43365646576 +40.50892719489 14.3659 13.9063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160675_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160675_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160678_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160678_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160687_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160687_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:44:51.34 +42:10:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 0.629 203620452432784256 071.21407176046 +42.16807609497 14.1741 13.5494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160688_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160688_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160689_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160689_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:53:21.64 +36:24:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.239 219831892390532608 058.34025537612 +36.40177116321 14.1101 13.5830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160692_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160692_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:38:43.18 +39:46:03.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160694_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160694_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160695_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160695_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160696_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160696_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160697_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160697_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160700_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160700_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160701_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160701_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160703_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160703_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160704_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160704_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160705_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160705_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160710_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160710_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160711_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160711_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160712_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160712_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160713_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160713_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160715_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160715_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160716_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160716_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160725_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160725_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160729_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160729_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160738_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160738_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160740_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160740_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:21:25.70 +41:52:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.895 228359464058455296 065.35681495460 +41.87164792605 11.4951 10.1506 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160741_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160741_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160742_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160742_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160743_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160743_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:36:34.26 +41:36:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.122 204004628666677632 069.14245818378 +41.60144416003 14.3963 13.7467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160747_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160747_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160751_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160751_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160755_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160755_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:59:25.44 +38:32:59.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160761_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160761_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:59:10.57 +40:15:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.345 200783574995309696 074.79471842971 +40.26054740777 13.9217 12.9244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160766_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160766_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160772_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160772_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:12:58.51 +34:42:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.899 176794224143375360 063.24433248551 +34.70808953580 14.5162 13.7150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160773_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160773_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160782_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160782_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:56:01.48 +40:10:08.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160785_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160785_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160793_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160793_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160794_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160794_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:41:47.42 +37:19:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 2.078 175502401055690368 070.44827415159 +37.31923929606 13.7928 12.7115 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160795_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160795_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160796_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160796_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160797_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160797_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160805_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160805_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:25:37.62 +42:18:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.997 228433784175177216 066.40740044540 +42.31105386906 14.4698 13.7754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160808_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160808_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:26:34.42 +40:55:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 2.387 228039639315517824 066.64381819671 +40.91818832888 14.5062 13.8804 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160821_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160821_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:25:51.53 +34:01:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 2.259 173179579662210688 066.46545325198 +34.02625191880 14.4796 13.6332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160830_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160830_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160835_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160835_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160852_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160852_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160859_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160859_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160860_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160860_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160891_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160891_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160893_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160893_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:12:47.87 +39:39:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 2.320 226276748515150336 063.20027917166 +39.65829269097 14.2903 13.6235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160899_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160899_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160919_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 160919_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10702_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 10702_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:32:15.36 +42:36:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 3.321 252257963465959680 068.06469160485 +42.60401941355 13.8810 11.3413 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86190_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 86190_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148852_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 148852_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:43:38.86 +42:40:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.337 243289350195028608 055.91145578725 +42.67031897942 12.1069 11.6914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158668_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 158668_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107029_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 107029_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22765_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 22765_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 05:00:01.51 +41:25:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.894 201699777419522432 075.00563335246 +41.42409886450 13.5023 12.9579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115519_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 115519_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:15:40.71 +35:31:59.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37420_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 37420_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08222_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 08222_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07097_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 07097_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:58:40.78 +42:17:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.912 201983107821992448 074.66915206022 +42.29234994440 13.3576 13.1005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116977_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 116977_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:49:34.34 +35:35:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.658 219880339620810240 057.39186918378 +35.59451011765 12.9629 12.0886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87160_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 87160_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94341_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 94341_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:51:17.02 +33:02:15.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12453_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 12453_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45725_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 45725_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128098_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 128098_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126163_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 126163_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65245_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 65245_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148156_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 148156_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:57:14.98 +41:53:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 5.667 201867998399665536 074.31033768277 +41.88367534695 13.4932 12.9809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52541_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 52541_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147906_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 147906_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 03:45:36.47 +34:50:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.958 218337862246417920 056.40228155650 +34.84645009579 14.0660 13.5130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27710_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 27710_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61976_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 61976_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
**** FOUND 04:29:15.08 +39:33:44.0 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30159_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
Preparing report for the candidate 30159_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44955_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019
The candidate 44955_fd_Per-05-Q2b1x1_2026-03-19_21-07-34_20.00sec_-15.00C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 13s
make_report_in_HTML.sh TOTAL: 169s
Prepared the HTML report for the field Per-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:29:15.07 +39:33:44.0
04:15:40.68 +35:31:59.3
03:42:34.79 +41:05:34.3
03:41:34.73 +41:05:57.2
03:47:51.39 +42:24:54.6
03:51:17.02 +33:02:15.5
04:59:32.61 +42:12:26.8
03:45:32.07 +34:51:31.7
04:29:17.92 +42:33:35.4
03:45:20.83 +41:42:39.4
03:43:19.67 +39:27:33.0
03:47:32.26 +42:45:41.3
03:41:21.09 +41:02:18.0
03:44:17.38 +42:09:08.9
03:43:38.12 +41:29:24.6
03:44:40.22 +41:24:56.8
03:47:30.37 +42:27:07.4
03:41:58.62 +40:15:22.1
03:47:52.39 +42:49:22.9
03:47:29.73 +42:33:17.4
03:43:14.80 +40:54:09.8
03:43:13.37 +39:03:41.7
03:43:20.92 +40:30:52.2
03:46:32.64 +41:30:32.9
03:42:47.44 +39:52:37.5
03:42:54.25 +42:21:53.7
03:41:16.75 +41:38:03.5
03:42:18.74 +42:23:14.7
03:42:53.63 +41:49:10.8
03:46:25.35 +42:33:38.1
03:43:21.08 +42:17:26.3
03:41:41.69 +41:30:55.2
03:47:34.56 +42:51:33.4
03:42:57.87 +41:37:04.9
03:42:31.75 +40:29:17.6
03:42:41.98 +40:21:49.2
03:43:36.35 +42:18:29.1
03:44:42.66 +42:16:54.9
03:46:09.03 +41:09:42.2
03:41:55.30 +42:04:28.5
03:42:16.48 +40:00:27.1
03:47:36.35 +42:26:39.5
03:43:27.46 +41:11:18.2
03:42:12.25 +39:31:12.8
03:40:42.65 +42:31:34.8
03:44:00.25 +41:43:08.6
03:42:03.24 +40:37:42.2
03:41:19.62 +42:31:52.4
03:44:19.70 +41:56:27.7
03:43:14.43 +39:40:13.2
03:41:45.24 +40:09:32.4
03:44:12.57 +41:12:06.0
03:43:28.85 +42:09:00.2
03:43:04.75 +40:19:37.2
03:42:04.33 +42:44:25.3
03:43:44.89 +41:26:42.1
03:43:14.71 +40:30:26.0
03:41:51.24 +40:38:29.1
03:42:24.08 +39:37:28.0
03:43:26.39 +41:59:31.5
03:42:27.96 +40:24:22.1
03:46:35.83 +41:42:42.3
03:41:22.32 +41:08:27.3
04:44:41.94 +41:22:54.0
03:55:21.98 +41:12:48.2
04:19:09.15 +40:45:43.7
04:50:00.77 +39:55:57.8
04:16:24.28 +39:25:45.6
04:16:01.32 +37:20:29.1
########### Completed Per-05-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 ####
03:42:34.79 +41:05:34.3
03:41:34.73 +41:05:57.2
03:47:51.39 +42:24:54.6
03:51:17.02 +33:02:15.5
04:29:15.07 +39:33:44.0
04:15:40.68 +35:31:59.3
03:45:20.83 +41:42:39.4
03:43:19.67 +39:27:33.0
03:47:32.26 +42:45:41.3
03:41:21.09 +41:02:18.0
03:44:17.38 +42:09:08.9
03:43:38.12 +41:29:24.6
03:44:40.22 +41:24:56.8
03:47:30.37 +42:27:07.4
03:41:58.62 +40:15:22.1
03:47:52.39 +42:49:22.9
03:47:29.73 +42:33:17.4
03:43:14.80 +40:54:09.8
03:43:13.37 +39:03:41.7
03:43:20.92 +40:30:52.2
03:46:32.64 +41:30:32.9
03:42:47.44 +39:52:37.5
03:42:54.25 +42:21:53.7
03:41:16.75 +41:38:03.5
03:42:18.74 +42:23:14.7
03:42:53.63 +41:49:10.8
03:46:25.35 +42:33:38.1
03:43:21.08 +42:17:26.3
03:41:41.69 +41:30:55.2
03:47:34.56 +42:51:33.4
03:42:57.87 +41:37:04.9
03:42:31.75 +40:29:17.6
03:42:41.98 +40:21:49.2
03:43:36.35 +42:18:29.1
03:44:42.66 +42:16:54.9
03:46:09.03 +41:09:42.2
03:41:55.30 +42:04:28.5
03:42:16.48 +40:00:27.1
03:47:36.35 +42:26:39.5
03:43:27.46 +41:11:18.2
03:42:12.25 +39:31:12.8
03:40:42.65 +42:31:34.8
03:44:00.25 +41:43:08.6
03:42:03.24 +40:37:42.2
03:41:19.62 +42:31:52.4
03:44:19.70 +41:56:27.7
03:43:14.43 +39:40:13.2
03:41:45.24 +40:09:32.4
03:44:12.57 +41:12:06.0
03:43:28.85 +42:09:00.2
03:43:04.75 +40:19:37.2
03:42:04.33 +42:44:25.3
03:43:44.89 +41:26:42.1
03:43:14.71 +40:30:26.0
03:41:51.24 +40:38:29.1
03:42:24.08 +39:37:28.0
03:43:26.39 +41:59:31.5
03:42:27.96 +40:24:22.1
03:46:35.83 +41:42:42.3
03:41:22.32 +41:08:27.3
03:45:32.07 +34:51:31.7
03:55:21.98 +41:12:48.2
04:59:32.61 +42:12:26.8
04:16:01.32 +37:20:29.1
04:29:17.92 +42:33:35.4
04:19:09.15 +40:45:43.7
04:16:24.28 +39:25:45.6
04:50:00.77 +39:55:57.8
04:44:41.94 +41:22:54.0
###################################################################################
03:42:34.79 +41:05:34.3 -- not an asteroid (will add it to exclusion list)
03:41:34.73 +41:05:57.2 -- not an asteroid (will add it to exclusion list)
03:47:51.39 +42:24:54.6 -- not an asteroid (will add it to exclusion list)
03:51:17.02 +33:02:15.5 -- not an asteroid (will add it to exclusion list)
04:29:15.07 +39:33:44.0 -- not an asteroid (will add it to exclusion list)
04:15:40.68 +35:31:59.3 -- not an asteroid (will add it to exclusion list)
03:45:20.83 +41:42:39.4 -- not an asteroid (will add it to exclusion list)
03:43:19.67 +39:27:33.0 -- not an asteroid (will add it to exclusion list)
03:47:32.26 +42:45:41.3 -- not an asteroid (will add it to exclusion list)
03:41:21.09 +41:02:18.0 -- not an asteroid (will add it to exclusion list)
03:44:17.38 +42:09:08.9 -- not an asteroid (will add it to exclusion list)
03:43:38.12 +41:29:24.6 -- not an asteroid (will add it to exclusion list)
03:44:40.22 +41:24:56.8 -- not an asteroid (will add it to exclusion list)
03:47:30.37 +42:27:07.4 -- not an asteroid (will add it to exclusion list)
03:41:58.62 +40:15:22.1 -- not an asteroid (will add it to exclusion list)
03:47:52.39 +42:49:22.9 -- not an asteroid (will add it to exclusion list)
03:47:29.73 +42:33:17.4 -- not an asteroid (will add it to exclusion list)
03:43:14.80 +40:54:09.8 -- not an asteroid (will add it to exclusion list)
03:43:13.37 +39:03:41.7 -- not an asteroid (will add it to exclusion list)
03:43:20.92 +40:30:52.2 -- not an asteroid (will add it to exclusion list)
03:46:32.64 +41:30:32.9 -- not an asteroid (will add it to exclusion list)
03:42:47.44 +39:52:37.5 -- not an asteroid (will add it to exclusion list)
03:42:54.25 +42:21:53.7 -- not an asteroid (will add it to exclusion list)
03:41:16.75 +41:38:03.5 -- not an asteroid (will add it to exclusion list)
03:42:18.74 +42:23:14.7 -- not an asteroid (will add it to exclusion list)
03:42:53.63 +41:49:10.8 -- not an asteroid (will add it to exclusion list)
03:46:25.35 +42:33:38.1 -- not an asteroid (will add it to exclusion list)
03:43:21.08 +42:17:26.3 -- not an asteroid (will add it to exclusion list)
03:41:41.69 +41:30:55.2 -- not an asteroid (will add it to exclusion list)
03:47:34.56 +42:51:33.4 -- not an asteroid (will add it to exclusion list)
03:42:57.87 +41:37:04.9 -- not an asteroid (will add it to exclusion list)
03:42:31.75 +40:29:17.6 -- not an asteroid (will add it to exclusion list)
03:42:41.98 +40:21:49.2 -- not an asteroid (will add it to exclusion list)
03:43:36.35 +42:18:29.1 -- not an asteroid (will add it to exclusion list)
03:44:42.66 +42:16:54.9 -- not an asteroid (will add it to exclusion list)
03:46:09.03 +41:09:42.2 -- not an asteroid (will add it to exclusion list)
03:41:55.30 +42:04:28.5 -- not an asteroid (will add it to exclusion list)
03:42:16.48 +40:00:27.1 -- not an asteroid (will add it to exclusion list)
03:47:36.35 +42:26:39.5 -- not an asteroid (will add it to exclusion list)
03:43:27.46 +41:11:18.2 -- not an asteroid (will add it to exclusion list)
03:42:12.25 +39:31:12.8 -- not an asteroid (will add it to exclusion list)
03:40:42.65 +42:31:34.8 -- not an asteroid (will add it to exclusion list)
03:44:00.25 +41:43:08.6 -- not an asteroid (will add it to exclusion list)
03:42:03.24 +40:37:42.2 -- not an asteroid (will add it to exclusion list)
03:41:19.62 +42:31:52.4 -- not an asteroid (will add it to exclusion list)
03:44:19.70 +41:56:27.7 -- not an asteroid (will add it to exclusion list)
03:43:14.43 +39:40:13.2 -- not an asteroid (will add it to exclusion list)
03:41:45.24 +40:09:32.4 -- not an asteroid (will add it to exclusion list)
03:44:12.57 +41:12:06.0 -- not an asteroid (will add it to exclusion list)
03:43:28.85 +42:09:00.2 -- not an asteroid (will add it to exclusion list)
03:43:04.75 +40:19:37.2 -- not an asteroid (will add it to exclusion list)
03:42:04.33 +42:44:25.3 -- not an asteroid (will add it to exclusion list)
03:43:44.89 +41:26:42.1 -- not an asteroid (will add it to exclusion list)
03:43:14.71 +40:30:26.0 -- not an asteroid (will add it to exclusion list)
03:41:51.24 +40:38:29.1 -- not an asteroid (will add it to exclusion list)
03:42:24.08 +39:37:28.0 -- not an asteroid (will add it to exclusion list)
03:43:26.39 +41:59:31.5 -- not an asteroid (will add it to exclusion list)
03:42:27.96 +40:24:22.1 -- not an asteroid (will add it to exclusion list)
03:46:35.83 +41:42:42.3 -- not an asteroid (will add it to exclusion list)
03:41:22.32 +41:08:27.3 -- not an asteroid (will add it to exclusion list)
03:45:32.07 +34:51:31.7 -- not an asteroid (will add it to exclusion list)
03:55:21.98 +41:12:48.2 -- not an asteroid (will add it to exclusion list)
04:59:32.61 +42:12:26.8 -- not an asteroid (will add it to exclusion list)
04:16:01.32 +37:20:29.1 -- not an asteroid (will add it to exclusion list)
04:29:17.92 +42:33:35.4 -- not an asteroid (will add it to exclusion list)
04:19:09.15 +40:45:43.7 -- not an asteroid (will add it to exclusion list)
04:16:24.28 +39:25:45.6 -- not an asteroid (will add it to exclusion list)
04:50:00.77 +39:55:57.8 -- not an asteroid (will add it to exclusion list)
04:44:41.94 +41:22:54.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:40:42.65 +42:31:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:16.75 +41:38:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:19.62 +42:31:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:21.09 +41:02:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:22.32 +41:08:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:34.73 +41:05:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:41.69 +41:30:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:45.24 +40:09:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:51.24 +40:38:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:55.30 +42:04:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:58.62 +40:15:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:03.24 +40:37:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:04.33 +42:44:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:12.25 +39:31:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:16.48 +40:00:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:18.74 +42:23:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:24.08 +39:37:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:27.96 +40:24:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:31.75 +40:29:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:34.79 +41:05:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:41.98 +40:21:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:47.44 +39:52:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:53.63 +41:49:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:54.25 +42:21:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:57.87 +41:37:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:04.75 +40:19:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:13.37 +39:03:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:14.43 +39:40:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:14.71 +40:30:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:14.80 +40:54:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:19.67 +39:27:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:20.92 +40:30:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:21.08 +42:17:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:26.39 +41:59:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:27.46 +41:11:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:28.85 +42:09:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:36.35 +42:18:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:38.12 +41:29:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:44.89 +41:26:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:00.25 +41:43:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:12.57 +41:12:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:17.38 +42:09:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:19.70 +41:56:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:40.22 +41:24:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:42.66 +42:16:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:20.83 +41:42:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:32.07 +34:51:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:09.03 +41:09:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:25.35 +42:33:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:32.64 +41:30:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:35.83 +41:42:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:29.73 +42:33:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:30.37 +42:27:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:32.26 +42:45:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:34.56 +42:51:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:36.35 +42:26:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:51.39 +42:24:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:52.39 +42:49:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:17.02 +33:02:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:21.98 +41:12:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:40.68 +35:31:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:16:01.32 +37:20:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:16:24.28 +39:25:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:19:09.15 +40:45:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:15.07 +39:33:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:17.92 +42:33:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:44:41.94 +41:22:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:00.77 +39:55:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:32.61 +42:12:26.8 -- 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)
03:40:42.65 +42:31:34.8 -- not a known variable star
03:41:16.75 +41:38:03.5 -- not a known variable star
03:41:19.62 +42:31:52.4 -- not a known variable star
03:41:21.09 +41:02:18.0 -- not a known variable star
03:41:22.32 +41:08:27.3 -- not a known variable star
03:41:34.73 +41:05:57.2 -- a known variable star
03:41:41.69 +41:30:55.2 -- not a known variable star
03:41:45.24 +40:09:32.4 -- not a known variable star
03:41:51.24 +40:38:29.1 -- not a known variable star
03:41:55.30 +42:04:28.5 -- not a known variable star
03:41:58.62 +40:15:22.1 -- not a known variable star
03:42:03.24 +40:37:42.2 -- a known variable star
03:42:04.33 +42:44:25.3 -- not a known variable star
03:42:12.25 +39:31:12.8 -- not a known variable star
03:42:16.48 +40:00:27.1 -- not a known variable star
03:42:18.74 +42:23:14.7 -- not a known variable star
03:42:24.08 +39:37:28.0 -- not a known variable star
03:42:27.96 +40:24:22.1 -- a known variable star
03:42:31.75 +40:29:17.6 -- not a known variable star
03:42:34.79 +41:05:34.3 -- not a known variable star
03:42:41.98 +40:21:49.2 -- not a known variable star
03:42:47.44 +39:52:37.5 -- not a known variable star
03:42:53.63 +41:49:10.8 -- not a known variable star
03:42:54.25 +42:21:53.7 -- not a known variable star
03:42:57.87 +41:37:04.9 -- a known variable star
03:43:04.75 +40:19:37.2 -- not a known variable star
03:43:13.37 +39:03:41.7 -- not a known variable star
03:43:14.43 +39:40:13.2 -- not a known variable star
03:43:14.71 +40:30:26.0 -- not a known variable star
03:43:14.80 +40:54:09.8 -- not a known variable star
03:43:19.67 +39:27:33.0 -- not a known variable star
03:43:20.92 +40:30:52.2 -- not a known variable star
03:43:21.08 +42:17:26.3 -- not a known variable star
03:43:26.39 +41:59:31.5 -- not a known variable star
03:43:27.46 +41:11:18.2 -- not a known variable star
03:43:28.85 +42:09:00.2 -- not a known variable star
03:43:36.35 +42:18:29.1 -- not a known variable star
03:43:38.12 +41:29:24.6 -- not a known variable star
03:43:44.89 +41:26:42.1 -- not a known variable star
03:44:00.25 +41:43:08.6 -- not a known variable star
03:44:12.57 +41:12:06.0 -- not a known variable star
03:44:17.38 +42:09:08.9 -- not a known variable star
03:44:19.70 +41:56:27.7 -- not a known variable star
03:44:40.22 +41:24:56.8 -- not a known variable star
03:44:42.66 +42:16:54.9 -- not a known variable star
03:45:20.83 +41:42:39.4 -- not a known variable star
03:45:32.07 +34:51:31.7 -- not a known variable star
03:46:09.03 +41:09:42.2 -- not a known variable star
03:46:25.35 +42:33:38.1 -- not a known variable star
03:46:32.64 +41:30:32.9 -- not a known variable star
03:46:35.83 +41:42:42.3 -- not a known variable star
03:47:29.73 +42:33:17.4 -- not a known variable star
03:47:30.37 +42:27:07.4 -- not a known variable star
03:47:32.26 +42:45:41.3 -- not a known variable star
03:47:34.56 +42:51:33.4 -- a known variable star
03:47:36.35 +42:26:39.5 -- not a known variable star
03:47:51.39 +42:24:54.6 -- not a known variable star
03:47:52.39 +42:49:22.9 -- not a known variable star
03:51:17.02 +33:02:15.5 -- a known variable star
03:55:21.98 +41:12:48.2 -- a known variable star
04:15:40.68 +35:31:59.3 -- a known variable star
04:16:01.32 +37:20:29.1 -- a known variable star
04:16:24.28 +39:25:45.6 -- a known variable star
04:19:09.15 +40:45:43.7 -- a known variable star
04:29:15.07 +39:33:44.0 -- a known variable star
04:29:17.92 +42:33:35.4 -- a known variable star
04:44:41.94 +41:22:54.0 -- a known variable star
04:50:00.77 +39:55:57.8 -- a known variable star
04:59:32.61 +42:12:26.8 -- a known variable star
Found 53 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
69 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 69 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461119.58819169 -observatory 500
22:37:26.88 -07:25:55.6 Mercury (1.2mag)
01:02:25.68 +05:41:22.2 Venus (-3.9mag)
23:00:30.20 -07:30:59.1 Mars (1.2mag)
07:04:38.59 +22:58:09.2 Jupiter (-2.3mag)
00:16:55.90 -00:28:52.4 Saturn (0.9mag)
03:42:47.93 +19:31:24.9 Uranus (5.8mag)
00:07:09.78 -00:38:51.3 Neptune (7.8mag)
20:31:55.40 -22:53:55.3 Pluto (14.5mag)
00:41:47.94 +07:41:23.7 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Mar 19 21:34 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461119.58819169:
07:04:29.58 +22:58:25.7 Io (5.6mag)
07:04:41.58 +22:57:59.7 Europa (5.7mag)
07:04:29.25 +22:58:18.9 Ganymede (5.2mag)
07:04:10.12 +22:58:53.5 Callisto (6.4mag)
07:08:40.02 +23:00:18.0 Himalia (15.2mag)
07:04:37.63 +22:58:08.0 Thebe (16.0mag)
07:08:13.78 +23:23:10.2 Elara (17.1mag)
07:01:43.05 +23:52:19.2 Pasiphae (17.2mag)
07:13:26.74 +22:52:26.4 Carme (18.3mag)
00:16:47.67 -00:28:41.4 Titan (8.8mag)
00:16:55.06 -00:28:46.9 Rhea (10.1mag)
00:17:26.32 -00:26:54.0 Iapetus (11.5mag)
00:17:09.98 -00:29:00.9 Hyperion (14.8mag)
00:18:50.51 -00:17:31.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 19 21:34 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461119.58819169:
12:42:13.29 +09:48:58.6 JWST
19:19:36.76 +12:56:13.4 Chandra
15:23:29.19 -59:23:39.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 19 21:34 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461119.58819169 -observatory 500
18:34:38.00 -27:25:17.6 14.1mag P/2010 H2 (Vales)
04:50:44.64 -71:05:08.0 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:40.83 +31:17:41.0 17.0mag C/2017 K2 (PANSTARRS)
17:29:28.95 +07:17:43.7 17.6mag C/2021 G2 (ATLAS)
23:01:12.05 +28:25:07.5 16.9mag C/2022 E2 (ATLAS)
03:59:33.30 +25:16:04.8 15.7mag C/2022 N2 (PANSTARRS)
09:01:58.85 +31:24:44.2 16.0mag C/2022 QE78 (ATLAS)
08:30:16.61 -03:17:27.6 17.2mag C/2022 R6 (PANSTARRS)
18:56:28.25 +16:12:49.1 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:26.70 -11:51:13.5 17.6mag P/2023 B1 (PANSTARRS)
09:25:17.89 -16:29:19.4 17.4mag C/2023 F3 (ATLAS)
21:20:19.59 +61:40:00.8 17.4mag C/2023 H5 (Lemmon)
19:33:25.57 -03:31:03.7 14.5mag C/2023 R1 (PANSTARRS)
21:35:34.09 +82:46:22.9 17.7mag C/2023 X2 (Lemmon)
06:15:42.86 +63:47:54.1 16.8mag C/2024 A1 (ATLAS)
04:03:26.94 +04:30:59.0 9.0mag C/2024 E1 (Wierzchos)
11:23:23.68 +02:33:00.1 18.0mag C/2024 G2 (ATLAS)
16:32:35.24 +02:01:18.9 17.5mag C/2024 G6 (ATLAS)
20:09:34.24 +08:33:24.7 14.9mag C/2024 J3 (ATLAS)
03:04:00.87 -26:48:49.1 16.5mag C/2024 T5 (ATLAS)
04:57:00.62 +52:53:51.9 17.6mag C/2025 J1 (Borisov)
15:16:12.43 +16:14:04.5 14.4mag C/2025 L1 (ATLAS)
02:47:23.62 -22:27:43.3 17.6mag C/2025 Q3 (ATLAS)
22:32:19.77 +18:57:09.2 12.6mag C/2025 R3 (PANSTARRS)
13:05:24.73 +01:15:05.7 17.7mag C/2025 Y1 (ATLAS)
02:12:00.61 -06:54:28.1 14.3mag C/2026 A1 (MAPS)
22:35:50.27 +30:46:00.6 13.7mag C/2026 B2 (Sun-Gao)
17:50:17.34 -10:52:00.8 13.4mag 10P/Tempel
15:27:12.68 +05:10:59.6 11.7mag 24P/Schaumasse
11:12:22.91 -02:30:58.4 15.6mag 29P/Schwassmann-Wachmann
17:42:43.05 -10:40:47.9 17.3mag 40P/Vaisala
10:45:38.10 -06:39:35.9 16.4mag 43P/Wolf-Harrington
01:07:35.25 +12:45:32.0 17.0mag 47P/Ashbrook-Jackson
06:27:22.37 +42:31:47.3 17.1mag 63P/Wild
22:52:54.99 -14:51:45.4 15.7mag 65P/Gunn
02:56:21.41 +10:56:31.0 15.9mag 76P/West-Kohoutek-Ikemura
00:07:35.92 +02:52:01.3 14.7mag 78P/Gehrels
21:35:35.48 -16:58:39.0 14.5mag 88P/Howell
00:58:27.62 +12:57:17.1 15.3mag 93P/Lovas
04:09:14.41 +30:37:27.1 16.5mag 123P/West-Hartley
08:07:33.18 +50:40:16.0 16.2mag 124P/Mrkos
01:53:01.57 +11:14:44.1 16.4mag 128P/Shoemaker-Holt
01:55:40.57 +10:54:09.9 17.4mag 131P/Mueller
23:16:06.51 +02:44:04.4 13.1mag 141P/Machholz
23:26:10.48 -04:43:17.5 13.1mag 141P-A/Machholz
22:27:31.08 -07:12:05.6 16.2mag 141P-D/Machholz
23:47:52.67 -14:33:58.6 15.5mag 162P/SidingSpring
10:39:59.69 +32:02:14.6 17.5mag 164P/Christensen
05:48:10.17 +24:44:28.7 17.5mag 198P/ODAS
15:34:30.00 -03:29:56.5 16.9mag 210P/Christensen
20:08:19.55 -17:44:22.2 17.1mag 218P/LINEAR
16:58:17.75 -16:45:12.0 16.3mag 235P/LINEAR
04:39:43.08 +31:52:42.5 16.3mag 240P/NEAT
07:29:44.82 -08:29:52.7 17.5mag 242P/Spahr
15:48:36.99 +05:02:10.9 17.7mag 391P/Kowalski
07:27:55.39 +21:05:30.3 17.5mag 450P/LONEOS
04:59:51.93 +46:40:37.3 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 19 21:34 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
-rw-r--r-- 1 apache apache 5.7K Mar 19 21:34 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 19 21:34 tocp_transients_list.txt