This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti
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 20.0803 2461119.5803 11.19 08:15:30.24 -29:36:52.5
248.57702 2.98975 galactic Pup Second-epoch detections are separated by 0.8" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J123.8815-29.6140 | 08:15:30.24 -29:36:52.5 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J123.8815-29.6140,2461119.5803,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J123.8815-29.6140 20260320.0803 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:30.24 -29:36:52.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 10.94 08:14:10.13 -29:36:56.1
248.41699 2.74754 galactic Pup Second-epoch detections are separated by 2.3" 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 | DocumentRef: VOTx1398302 | 08:14:09.56 -29:36:57.6 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx1398302,2461119.5803,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx1398302 20260320.0803 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:10.13 -29:36:56.1 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
BP CMa,2461119.5803,10.47,0.05,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
BP CMa 20260320.0803 10.47CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:15:20.11 -22:00:50.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.34 08:15:12.41 -30:25:31.8
249.21670 2.48629 galactic Pup Second-epoch detections are separated by 3.0" and 2.5 pix
The object was found in VSX15" ASAS J081514-3025.6
Type: M
# Max. Min./Amp. JD0 Period
10.900 V 15.700 V 2452972.00000 287.000000000000 M6
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J081514-3025.6,2461119.5803,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J081514-3025.6 20260320.0803 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:12.41 -30:25:31.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
CD Pup,2461119.5803,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CD Pup 20260320.0803 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:42.18 -24:17:49.2 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
NSV 3807,2461119.5803,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 3807 20260320.0803 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:54:32.25 -23:50:21.0 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.55 07:42:27.37 -27:32:06.7
243.00057 -2.09565 galactic Pup Second-epoch detections are separated by 0.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx1415163 | 07:42:27.37 -27:32:06.7 (user input) | (GCVS) | (GCVS) | (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx1415163,2461119.5803,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx1415163 20260320.0803 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:42:27.37 -27:32:06.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.50 07:21:50.25 -27:56:46.5
241.17524 -6.29886 galactic CMa Second-epoch detections are separated by 0.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J110.4587-27.9464 | 07:21:50.11 -27:56:47.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.671+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J110.4587-27.9464,2461119.5803,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.4587-27.9464 20260320.0803 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:21:50.25 -27:56:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.54 07:29:45.37 -29:15:30.9
243.15699 -5.37358 galactic Pup Second-epoch detections are separated by 1.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5611568389349752576 | 07:29:44.71 -29:15:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5611568389349752576,2461119.5803,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5611568389349752576 20260320.0803 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:29:45.37 -29:15:30.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.59 07:41:33.84 -27:05:29.6
242.51668 -2.04832 galactic Pup Second-epoch detections are separated by 1.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J115.3910-27.0855 | 07:41:33.83 -27:05:30.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.069+/-0.030 (A)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J115.3910-27.0855,2461119.5803,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J115.3910-27.0855 20260320.0803 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:41:33.84 -27:05:29.6 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
GDS_J0758256-300853,2461119.5803,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0758256-300853 20260320.0803 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:58:25.26 -30:08:48.9 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.93 08:04:06.19 -29:08:29.5
246.82748 1.16343 galactic Pup Second-epoch detections are separated by 3.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5597520792588416000 | 08:04:03.61 -29:08:00.3 (Gaia DR3) | E (local) | F (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5597520792588416000,2461119.5803,12.93,0.05,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 5597520792588416000 20260320.0803 12.93CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:06.19 -29:08:29.5 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.90 08:10:58.84 -30:28:15.6
248.75269 1.70100 galactic Pup Second-epoch detections are separated by 3.2" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5596351251501308416 | 08:10:58.28 -30:28:18.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5596351251501308416,2461119.5803,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5596351251501308416 20260320.0803 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:58.84 -30:28:15.6 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.75 08:12:25.40 -30:23:54.8
248.86260 2.00081 galactic Pup Second-epoch detections are separated by 5.1" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5596439697776459136 | 08:12:24.92 -30:23:55.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5596439697776459136,2461119.5803,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 5596439697776459136 20260320.0803 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:12:25.40 -30:23:54.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.73 08:13:17.19 -27:45:26.4
246.75705 3.60990 galactic Pup Second-epoch detections are separated by 2.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J123.3101-27.7575 | 08:13:16.45 -27:45:30.1 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J123.3101-27.7575,2461119.5803,12.73,0.05,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 J123.3101-27.7575 20260320.0803 12.73CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:17.19 -27:45:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.53 08:10:23.15 -30:58:25.2
249.10401 1.31933 galactic Pup Second-epoch detections are separated by 0.7" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5596298616692334976 | 08:10:22.37 -30:58:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5596298616692334976,2461119.5803,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5596298616692334976 20260320.0803 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:23.15 -30:58:25.2 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.65 08:13:20.58 -27:40:23.1
246.69341 3.66664 galactic Pup Second-epoch detections are separated by 1.1" 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 | Gaia DR3 5693827698956897152 | 08:13:19.74 -27:40:25.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.108+/-0.203 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5693827698956897152,2461119.5803,12.65,0.05,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
Gaia DR3 5693827698956897152 20260320.0803 12.65CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:20.58 -27:40:23.1 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.52 08:11:39.36 -29:21:30.4
247.90097 2.43224 galactic Pup Second-epoch detections are separated by 1.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J122.8998-29.3583 | 08:11:38.85 -29:21:32.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J122.8998-29.3583,2461119.5803,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J122.8998-29.3583 20260320.0803 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:39.36 -29:21:30.4 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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 5692878103166922496,2461119.5803,12.40,0.05,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 5692878103166922496 20260320.0803 12.40CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:40.35 -28:38:19.2 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.37 08:15:39.65 -29:58:15.6
248.89276 2.82018 galactic Pup Second-epoch detections are separated by 3.1" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5644512339008750976 | 08:15:39.11 -29:58:19.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5644512339008750976,2461119.5803,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5644512339008750976 20260320.0803 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:39.65 -29:58:15.6 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.26 08:15:04.39 -27:15:09.0
246.55352 4.21865 galactic Pup Second-epoch detections are separated by 5.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J123.7516-27.2516 | 08:15:03.81 -27:15:10.7 (Gaia DR3) | SINE (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J123.7516-27.2516,2461119.5803,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J123.7516-27.2516 20260320.0803 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:04.39 -27:15:09.0 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.46 08:14:28.76 -30:36:59.2
249.28888 2.25005 galactic Pup Second-epoch detections are separated by 1.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5548380422485764352 | 08:14:29.31 -30:36:58.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5548380422485764352,2461119.5803,12.46,0.05,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 5548380422485764352 20260320.0803 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:28.76 -30:36:59.2 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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 5693000492552356480,2461119.5803,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5693000492552356480 20260320.0803 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:58.50 -28:10:07.3 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.07 08:13:35.69 -29:35:18.6
248.32545 2.65843 galactic Pup Second-epoch detections are separated by 4.3" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J123.4039-29.5831 | 08:13:34.83 -29:35:20.9 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J123.4039-29.5831,2461119.5803,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J123.4039-29.5831 20260320.0803 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:35.69 -29:35:18.6 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.23 08:10:21.54 -30:57:25.8
249.08705 1.32352 galactic Pup Second-epoch detections are separated by 1.9" 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 | Gaia DR3 5596301567319674112 | 08:10:20.76 -30:57:25.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8II 1971PW&SO...1a...1S LS 979
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5596301567319674112,2461119.5803,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5596301567319674112 20260320.0803 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:21.54 -30:57:25.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.14 08:15:25.43 -29:25:43.6
248.41252 3.07832 galactic Pup Second-epoch detections are separated by 3.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5692580410379472128 | 08:15:24.96 -29:25:46.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5692580410379472128,2461119.5803,12.14,0.05,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
Gaia DR3 5692580410379472128 20260320.0803 12.14CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:25.43 -29:25:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.12 08:14:04.96 -30:11:25.8
248.88636 2.41435 galactic Pup Second-epoch detections are separated by 1.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5596464230630634240 | 08:14:06.08 -30:11:27.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5596464230630634240,2461119.5803,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5596464230630634240 20260320.0803 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:04.96 -30:11:25.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.08 08:14:15.44 -30:30:36.4
249.17377 2.26908 galactic Pup Second-epoch detections are separated by 3.3" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5548417153047743104 | 08:14:16.03 -30:30:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5548417153047743104,2461119.5803,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5548417153047743104 20260320.0803 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:15.44 -30:30:36.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.01 08:13:52.40 -29:10:34.8
248.01470 2.93633 galactic Pup Second-epoch detections are separated by 2.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J123.4551-29.1846 | 08:13:51.77 -29:10:38.2 (Gaia DR3) | DBH (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J123.4551-29.1846,2461119.5803,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J123.4551-29.1846 20260320.0803 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:52.40 -29:10:34.8 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.93 08:12:34.02 -30:39:51.3
249.10170 1.88061 galactic Pup Second-epoch detections are separated by 5.1" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5548388050348173440 | 08:12:34.63 -30:39:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5548388050348173440,2461119.5803,11.93,0.05,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 5548388050348173440 20260320.0803 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:12:34.02 -30:39:51.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.85 08:15:39.82 -29:39:00.5
248.62592 2.99887 galactic Pup Second-epoch detections are separated by 1.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5692563848998183680 | 08:15:40.64 -29:39:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5692563848998183680,2461119.5803,11.85,0.05,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 5692563848998183680 20260320.0803 11.85CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:39.82 -29:39:00.5 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.55 08:15:07.52 -29:22:49.4
248.33610 3.05103 galactic Pup Second-epoch detections are separated by 0.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J123.7872-29.3751 | 08:15:06.97 -29:22:51.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J123.7872-29.3751,2461119.5803,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J123.7872-29.3751 20260320.0803 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:07.52 -29:22:49.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.24 08:15:11.56 -29:39:38.4
248.57785 2.90790 galactic Pup Second-epoch detections are separated by 0.8" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5692564330034654464 | 08:15:11.07 -29:39:40.3 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5692564330034654464,2461119.5803,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5692564330034654464 20260320.0803 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:11.56 -29:39:38.4 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.20 08:12:30.88 -20:53:56.0
240.88510 7.20254 galactic Pup Second-epoch detections are separated by 3.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASAS J081233-2053.6 | 08:12:33.30 -20:53:39.7 (Gaia DR3) | MISC (local) | 2452916.30000 (local) | Gaia3var=VARIABLE SpType: M6 1993yCat.3170....0M IRAS 08103-2044
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J081233-2053.6,2461119.5803,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J081233-2053.6 20260320.0803 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:12:30.88 -20:53:56.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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 5548287646884150400,2461119.5803,12.30,0.05,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
Gaia DR3 5548287646884150400 20260320.0803 12.30CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:12:38.48 -30:54:27.3 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.55 08:15:02.68 -30:30:40.2
249.26864 2.40969 galactic Pup Second-epoch detections are separated by 1.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5548406157931251968 | 08:15:01.79 -30:30:38.1 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5548406157931251968,2461119.5803,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5548406157931251968 20260320.0803 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:02.68 -30:30:40.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.79 07:49:23.64 -26:35:12.6
242.95471 -0.28378 galactic Pup Second-epoch detections are separated by 5.4" and 1.8 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 J117.3390-26.5845 | 07:49:23.64 -26:35:12.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J117.3390-26.5845,2461119.5803,12.79,0.05,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 J117.3390-26.5845 20260320.0803 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:49:23.64 -26:35:12.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
GDS_J0753219-310453,2461119.5803,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0753219-310453 20260320.0803 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:53:21.85 -31:04:52.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.87 07:42:36.49 -30:47:11.3
245.84635 -3.67506 galactic Pup Second-epoch detections are separated by 2.4" and 2.7 pix
The object was found in VSX 4" GDS_J0742363-304714
Type: M
# Max. Min./Amp. JD0 Period
12.000 V < 14.500 V 2453720.00000 255.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0742363-304714,2461119.5803,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0742363-304714 20260320.0803 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:42:36.49 -30:47:11.3 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
GDS_J0810215-295827,2461119.5803,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0810215-295827 20260320.0803 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:20.65 -29:58:23.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J071144.79-263327.3,2461119.5803,13.23,0.05,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
ASASSN-V J071144.79-263327.3 20260320.0803 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:11:44.91 -26:33:29.9 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
GDS_J0751291-292822,2461119.5803,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0751291-292822 20260320.0803 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:51:29.23 -29:28:21.0 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.16 07:05:26.16 -29:16:26.7
240.75370 -10.11261 galactic CMa Second-epoch detections are separated by 1.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.3501-29.2761 | 07:05:26.06 -29:16:27.0 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.609+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.3501-29.2761,2461119.5803,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3501-29.2761 20260320.0803 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:05:26.16 -29:16:26.7 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
ASAS J072910-2653.3,2461119.5803,12.30,0.05,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
ASAS J072910-2653.3 20260320.0803 12.30CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:29:10.59 -26:53:21.7 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.55 07:09:33.05 -30:08:53.2
241.94635 -9.68620 galactic CMa Second-epoch detections are separated by 1.1" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:09:33.05 -30:08:53.2 (user input) | T | P | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.5803,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0803 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:09:33.05 -30:08:53.2 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.5803,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0803 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:07:15.27 -28:23:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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 5609343394433693056,2461119.5803,11.64,0.05,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
Gaia DR3 5609343394433693056 20260320.0803 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:07:10.58 -29:12:07.9 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
BT CMa,2461119.5803,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BT CMa 20260320.0803 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:19:15.11 -21:07:56.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
ASAS J080744-2948.0,2461119.5803,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J080744-2948.0 20260320.0803 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:43.24 -29:47:57.8 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.01 08:14:11.81 -30:14:03.1
248.93645 2.41076 galactic Pup Second-epoch detections are separated by 0.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J123.5464-30.2454 | 08:14:11.13 -30:14:03.9 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J123.5464-30.2454,2461119.5803,11.01,0.05,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
ATO J123.5464-30.2454 20260320.0803 11.01CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:11.81 -30:14:03.1 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
EG Pup,2461119.5803,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EG Pup 20260320.0803 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:36:07.93 -26:30:16.5 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.35 07:07:13.76 -29:29:29.7
241.12430 -9.85434 galactic CMa Second-epoch detections are separated by 1.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.7997-29.4973 | 07:07:13.74 -29:29:29.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.278+/-0.033 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.7997-29.4973,2461119.5803,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.7997-29.4973 20260320.0803 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:07:13.76 -29:29:29.7 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.40 08:13:09.89 -22:21:16.0
242.19979 6.54086 galactic Pup Second-epoch detections are separated by 3.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5700584202202449664 | 08:13:10.57 -22:21:13.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5700584202202449664,2461119.5803,12.40,0.05,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 5700584202202449664 20260320.0803 12.40CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:09.89 -22:21:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
ASAS J074544-2812.5,2461119.5803,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J074544-2812.5 20260320.0803 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:43.92 -28:12:34.3 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 10.41 07:06:12.34 -30:23:31.4
241.85236 -10.44291 galactic CMa Second-epoch detections are separated by 0.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5604694178233997824 | 07:06:12.33 -30:23:31.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.662+/-0.050 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5604694178233997824,2461119.5803,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5604694178233997824 20260320.0803 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:06:12.34 -30:23:31.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.51 08:09:47.83 -29:59:22.5
248.20952 1.74939 galactic Pup Second-epoch detections are separated by 2.2" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5596519511139319936 | 08:09:47.35 -29:59:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5596519511139319936,2461119.5803,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5596519511139319936 20260320.0803 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:09:47.83 -29:59:22.5 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-45_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.65 08:15:38.01 -30:49:16.0
249.59701 2.34293 galactic Pup Second-epoch detections are separated by 1.3" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5548347162258655616 | 08:15:37.21 -30:49:12.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5548347162258655616,2461119.5803,11.65,0.05,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
Gaia DR3 5548347162258655616 20260320.0803 11.65CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:38.01 -30:49:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
ASAS J080125-2559.3,2461119.5803,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J080125-2559.3 20260320.0803 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:01:24.42 -25:59:16.1 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 11.84 07:16:58.03 -30:36:18.7
243.07710 -8.45306 galactic CMa Second-epoch detections are separated by 0.9" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5605247228285151104 | 07:16:58.18 -30:36:17.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.100+/-0.030 (A)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5605247228285151104,2461119.5803,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5605247228285151104 20260320.0803 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:16:58.03 -30:36:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
DO Pup,2461119.5803,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DO Pup 20260320.0803 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:09:05.97 -21:49:26.8 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_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
ET Pup,2461119.5803,10.42,0.05,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
ET Pup 20260320.0803 10.42CV 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:54:36.97 -28:05:00.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0803 2461119.5803 12.12 08:13:18.38 -30:36:38.3
249.14453 2.04288 galactic Pup Second-epoch detections are separated by 6.7" 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 | Large-amplitude variable Gaia DR2 5548392207876724224 | 08:13:18.11 -30:36:37.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 5548392207876724224,2461119.5803,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 5548392207876724224 20260320.0803 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:18.38 -30:36:38.3 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J071743.56-301051.2,2461119.5803,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J071743.56-301051.2 20260320.0803 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:17:44.55 -30:10:38.4 ;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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.72731285 09.01.2026 05:27:09.830 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
First image: 2461049.72731285 09.01.2026 05:27:09.830 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
Last image: 2461119.58051663 20.03.2026 01:55:46.637 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 53
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.31
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): 23618
Objects passed selection criteria: 23599
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: 22378.2
Average stars matched: 21845.5 (97.6193 %)
Memory usage VmPeak: 127392 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 22:09:54 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.72731285 09.01.2026 05:27:09.830 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
First image: 2461049.72731285 09.01.2026 05:27:09.830 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
Last image: 2461119.58051663 20.03.2026 01:55:46.637 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 543
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.02
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: 168 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): 207783
Objects passed selection criteria: 207336
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 187663
Average stars matched: 182121 (97.0468 %)
Memory usage VmPeak: 1968404 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 22:16:44 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
SExtractor catalog cache: saved Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat to cache
SExtractor catalog cache: saved Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.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: 2461119.58002206
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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits exists and is non-empty
Saving wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits to local_wcs_cache/
'wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits' -> 'local_wcs_cache/wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits'
wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits exists and is non-empty
Saving wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits to local_wcs_cache/
'wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits' -> 'local_wcs_cache/wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits'
wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits exists and is non-empty
Saving wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits to local_wcs_cache/
'wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits' -> 'local_wcs_cache/wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits'
wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits exists and is non-empty
Saving wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits to local_wcs_cache/
'wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits' -> 'local_wcs_cache/wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits'
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:40:43.459 -26:00:36.38
Second-epoch image center 07:40:47.855 -25:59:54.44
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:40:43.459 -26:00:36.38
Second-epoch image center 07:40:46.776 -25:59:55.37
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 07:40:47.855 -25:59:54.44
Second-epoch second image center 07:40:46.776 -25:59:55.37
Angular distance between the image centers 0.00405 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits &> /tmp/tmp.DaX69CDyAI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits &> /tmp/tmp.axD1eBn9Yk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits &> /tmp/tmp.VTplqjw1GR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits &> /tmp/tmp.rj9EYNfjFl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
Calibrating the magnitude scale
Found non-empty wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits and wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits and wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat
Found non-empty wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits and wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat
The reference image (wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits) and catalog (wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat) found
'wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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 1434 out of 24549 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.794999
a=0.000000 b=1.000000 c=22.794999
From vast_summary.log: estimated ref. image limiting mag.: -8.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 47 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
2.1 pix Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
2.6 pix fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
2.6 pix fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
Limiting magnitude estimates:
14.5 mag. Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
14.5 mag. Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
14.1 mag. fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
14.1 mag. fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.DaX69CDyAI (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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits' -> 'wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
Checking if the catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
WCS catalog name: wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2532, passed=24549
Got 24549 stars (including 21982 good ones) from the SExtractor catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat
util/solve_plate_with_UCAC5 got 24549 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 621 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: 5.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 650 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.54"
Estimated accuracy of the plate solution: 3.92"
Excluding outliers - 575 stars left (next iteration limit 594)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits -region wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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.axD1eBn9Yk (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/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits' -> 'wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
WCS-calibrated image found: wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
Checking if the catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
WCS catalog name: wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2529, passed=24619
Got 24619 stars (including 22058 good ones) from the SExtractor catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat
util/solve_plate_with_UCAC5 got 24619 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 914 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 905 stars left (next iteration limit 994)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits -region wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.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.VTplqjw1GR (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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
Checking if the catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat corresponding to the image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat corresponding to the image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
WCS catalog name: wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1526, passed=20211
Got 20211 stars (including 18673 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat
util/solve_plate_with_UCAC5 got 20211 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 892 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: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.87"
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 892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.88"
Estimated accuracy of the plate solution: 1.06"
Excluding outliers - 878 stars left (next iteration limit 966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits -region wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.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.rj9EYNfjFl (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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
Checking if the catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat corresponding to the image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat corresponding to the image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
WCS catalog name: wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1689, passed=20646
Got 20646 stars (including 18938 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat
util/solve_plate_with_UCAC5 got 20646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 894 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: 0.94"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.89"
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 894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.89"
Estimated accuracy of the plate solution: 1.02"
Excluding outliers - 881 stars left (next iteration limit 971)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits -region wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits'
Saving fully-calibrated image wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits'
Saving fully-calibrated image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits'
Saving fully-calibrated image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits'
Preparing the HTML report for the field Pup-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out31850.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31852.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31865.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31867.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31869.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31872.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31873.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31874.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31890.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31898.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out31828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31891.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 119s
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: 8s
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Considering the candidate 31828_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 31828_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 31831_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 31831_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 31835_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31835_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:18:42.28 -24:58:12.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31836_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31836_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:10:20.83 -23:00:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31837_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31837_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:54:36.93 -28:05:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.43, MAG_FAINT_SEARCH_LIMIT=11.41)GAIADR2_OUTPUT=# 4.178 5600692436944565888 118.65498947650 -28.08285577457 8.4781 7.1038 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31838_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31838_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:24:11.70 -29:16:30.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31839_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 31839_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 31840_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31840_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:23:59.67 -29:20:08.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31841_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31841_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:49:22.80 -24:53:27.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31842_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31842_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:13:43.37 -21:26:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.65, MAG_FAINT_SEARCH_LIMIT=11.63)GAIADR2_OUTPUT=# 2.040 2928379041101931264 108.43023758736 -21.44955738481 10.7455 10.0495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31843_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31843_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:18:42.60 -24:55:50.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31844_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31844_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:13:57.42 -30:19:35.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31845_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31845_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:36:07.83 -26:30:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 0.614 5612531256605718272 114.03278739121 -26.50468823954 11.1275 9.6904 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31846_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31846_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:19:15.05 -21:07:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 3.328 2929707422949867264 109.81204133678 -21.13137195322 11.6293 9.9274 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31848_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31848_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:23:23.10 -27:47:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 4.918 5612710820599728128 110.84778651134 -27.79822184199 11.1277 10.9228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31849_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 31849_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 31850_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31850_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:34:32.42 -24:03:28.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)
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Considering the candidate 31851_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31851_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:59:08.74 -22:26:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31852_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31852_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:35:06.38 -27:59:30.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)
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Considering the candidate 31853_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31853_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:43:40.91 -28:19:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 0.251 5599929582043772288 115.92053697883 -28.33063123559 10.8657 9.9574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31854_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31854_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:21:57.84 -29:07:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31855_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31855_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:43:38.70 -26:19:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 2.021 5613897773458277120 115.91063827988 -26.31725982195 11.5402 11.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31856_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31856_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:02:09.36 -24:51:57.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)
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Considering the candidate 31858_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31858_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:45:02.20 -25:37:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 0.781 5613995458188821504 116.25911070043 -25.61879444331 11.3255 10.9632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31859_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31859_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:39:02.45 -25:27:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 1.711 5614153238111093120 114.75994125573 -25.45168732302 11.4116 11.3830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31861_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31861_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:37:50.83 -25:51:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 1.227 5614105035704618880 114.46143659033 -25.86379810435 11.6632 11.6621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31863_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31863_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:44:36.29 -23:53:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 1.220 5614817862835644032 116.15106125081 -23.89392228688 11.4490 11.3463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31865_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31865_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:45:34.34 -27:16:13.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31866_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 31866_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31867_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31867_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:41:28.48 -26:30:57.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31869_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31869_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:42:59.16 -26:27:00.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31872_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31872_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:40:58.83 -28:11:38.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31873_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31873_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:41:44.16 -26:56:34.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31874_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31874_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:26:13.77 -29:51:35.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31876_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 31876_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31878_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31878_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:36:13.44 -27:07:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.165 5612473188647069696 114.05634656346 -27.12029110661 11.3739 11.1879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31879_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 31879_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31880_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 31880_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31883_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 31883_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31890_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31890_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:33:46.81 -25:29:39.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31891_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 31891_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31892_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31892_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:42:12.92 -24:41:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 1.363 5614670111651708672 115.55376861118 -24.68934614414 11.5389 11.4753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31897_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31897_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:43:37.10 -28:59:23.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31898_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31898_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:41:31.55 -27:15:21.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31900_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31900_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:32:09.16 -26:58:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 0.653 5612454565670404736 113.03822793850 -26.97642294027 11.3943 10.9296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31920_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 31920_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:06:14.44 -28:38:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 0.797 5609564391969776256 106.55993263504 -28.64327720719 11.2458 10.5332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03314_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 03314_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:12:02.67 -29:28:13.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 129s
Prepared the HTML report for the field Pup-02-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 ####
08:15:30.24 -29:36:52.5
08:14:10.13 -29:36:56.1
07:15:20.11 -22:00:50.1
08:15:12.41 -30:25:31.8
08:13:42.18 -24:17:49.2
07:54:32.25 -23:50:21.0
07:42:27.37 -27:32:06.7
07:21:50.25 -27:56:46.5
07:29:45.37 -29:15:30.9
07:41:33.84 -27:05:29.6
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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
SExtractor catalog cache: saved Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat to cache
SExtractor catalog cache: saved Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
Creating symlink local_wcs_cache/wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
Creating symlink local_wcs_cache/wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
Creating symlink local_wcs_cache/wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits exists and is non-empty
wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits exists and is non-empty
wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits exists and is non-empty
wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits exists and is non-empty
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:40:43.459 -26:00:36.38
Second-epoch image center 07:40:47.855 -25:59:54.44
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:40:43.459 -26:00:36.38
Second-epoch image center 07:40:46.776 -25:59:55.37
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 07:40:47.855 -25:59:54.44
Second-epoch second image center 07:40:46.776 -25:59:55.37
Angular distance between the image centers 0.00405 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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits &> /tmp/tmp.wYSlEZl9Sj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits &> /tmp/tmp.B5oEV8Lrzi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits &> /tmp/tmp.QVcIdou2bv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits &> /tmp/tmp.E6w8YVdDpn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
Calibrating the magnitude scale
Found non-empty wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits and wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits and wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat
Found non-empty wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits and wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat
The reference image (wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits) and catalog (wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat) found
'wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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 2433 out of 225162 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.517885
a=0.000000 b=1.000000 c=22.517885
From vast_summary.log: estimated ref. image limiting mag.: -8.02
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.50
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 444 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
1.9 pix Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
2.5 pix fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
2.4 pix fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
Limiting magnitude estimates:
14.5 mag. Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
14.5 mag. Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
14.1 mag. fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
14.1 mag. fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.4 (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.wYSlEZl9Sj (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/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits' -> 'wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
Checking if the catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
WCS catalog name: wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=61, blended=30068, passed=225101
Got 225101 stars (including 194663 good ones) from the SExtractor catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat
util/solve_plate_with_UCAC5 got 225101 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 617 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: 5.18"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.24"
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 649 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.23"
Estimated accuracy of the plate solution: 4.26"
Excluding outliers - 570 stars left (next iteration limit 584)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits -region wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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.B5oEV8Lrzi (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/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits' -> 'wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
WCS-calibrated image found: wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
Checking if the catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
WCS catalog name: wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=30182, passed=224219
Got 224219 stars (including 193668 good ones) from the SExtractor catalog wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat
util/solve_plate_with_UCAC5 got 224219 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 905 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 898 stars left (next iteration limit 987)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits -region wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.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.QVcIdou2bv (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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
Checking if the catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat corresponding to the image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat corresponding to the image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
WCS catalog name: wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=17049, passed=149161
Got 149161 stars (including 131980 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat
util/solve_plate_with_UCAC5 got 149161 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 888 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: 0.82"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.81"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.81"
Estimated accuracy of the plate solution: 0.95"
Excluding outliers - 874 stars left (next iteration limit 962)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits -region wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.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.E6w8YVdDpn (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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
Checking if the catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat corresponding to the image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat corresponding to the image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
WCS catalog name: wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=18204, passed=156393
Got 156393 stars (including 138035 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat
util/solve_plate_with_UCAC5 got 156393 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 897 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: 0.83"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.81"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.81"
Estimated accuracy of the plate solution: 0.94"
Excluding outliers - 884 stars left (next iteration limit 974)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits -region wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.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_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/wcs_Pup-02-Q2b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits
Saving fully-calibrated image wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/wcs_Pup-02-Q2b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits
Saving fully-calibrated image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-03_20.00sec_-15.00C_LIGHT_0006.fits
Saving fully-calibrated image wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.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_Pup-02-Q2b1x1_215951_TTUQ2b1x1_22328_Sqd4SYti/wcs_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007.fits
Preparing the HTML report for the field Pup-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out08511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out11051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out172952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out237496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out238104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out255510.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out255867.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out255991.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out04449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out186264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out224372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out238826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95156.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 79s
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: 27s
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Considering the candidate 255318_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255318_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255322_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255322_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:51:04.44 -23:59:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.608 5710643427931063168 117.76822147430 -23.99317251868 13.8048 13.2467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255323_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255323_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:42:51.67 -23:16:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.807 5615652082923282048 115.71537334882 -23.27335939111 14.3369 13.9049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255329_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255329_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:18:37.94 -21:39:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.500 2929618328145312000 109.65805398866 -21.65216405820 13.7420 13.4773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255335_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255335_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 255336_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255336_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:40:16.37 -22:41:26.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)
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Considering the candidate 255337_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255337_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 255343_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255343_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:46:21.21 -26:36:02.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 255344_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255344_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:42:42.60 -21:44:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.074 5712076916216665216 115.67721271118 -21.74535593151 14.0962 13.6496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255355_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255355_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:39:36.92 -23:11:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.047 5615773475877465088 114.90354805732 -23.18647684701 13.7840 13.4093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255356_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255356_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:50:12.32 -22:33:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.528 5711082717185512064 117.55051392300 -22.56481734337 14.0761 13.6031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255358_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255358_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:44:15.56 -22:54:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.742 5615699430643722240 116.06460521483 -22.90354702139 13.6981 13.2124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255363_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255363_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:55:33.86 -25:36:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.537 5602175781226097664 118.89276960423 -25.61290760212 13.5354 13.2847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255371_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255371_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:55:25.86 -21:01:34.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255376_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255376_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:38:27.56 -22:05:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.719 5618978861508179200 114.61435951236 -22.09832652760 13.5024 12.6685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255377_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255377_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:51:37.59 -26:24:43.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255378_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255378_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:35:02.09 -24:28:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.464 5615290618475216512 113.75863593101 -24.48045672615 13.3640 12.8894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255382_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255382_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:15:39.12 -27:28:51.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255392_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255392_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:59:45.47 -25:16:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 5.756 5698229357542613760 119.93812543013 -25.27064383784 13.4423 12.7459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255396_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255396_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:56:49.89 -22:13:27.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255397_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255397_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:20:20.85 -27:01:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.409 5612996831061709824 110.08696218340 -27.02216701060 13.1772 12.4032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255411_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255411_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:30:15.81 -21:12:57.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)
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Considering the candidate 255415_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255415_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:11:40.31 -22:49:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.793 5699724658989682432 122.91778256064 -22.82017692371 13.0149 12.3168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255418_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255418_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:42:46.44 -25:08:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.746 5614224092198494976 115.69333343396 -25.13378088438 13.6989 13.3395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255419_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255419_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 255424_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255424_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:55:26.83 -23:31:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.637 5710733278644881408 118.86160422040 -23.52881861518 13.3601 12.4167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255431_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255431_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:35:26.04 -24:56:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.046 5614989146132906880 113.85801774087 -24.94872416306 13.5920 13.1811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255432_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255432_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:12:18.38 -29:09:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.483 5606377496180717184 108.07649015829 -29.15624545383 13.4857 13.3409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255442_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255442_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:53:56.63 -21:16:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.013 5712316506669767680 118.48508211237 -21.27259371632 12.9757 11.8016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255443_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255443_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:54:18.21 -23:06:34.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 255446_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255446_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:50:47.40 -24:03:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.463 5710642672016883840 117.69773425688 -24.06124341690 13.5804 13.2907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255450_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255450_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:44:55.41 -24:40:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.955 5614635172111823232 116.23128491437 -24.68311754355 13.5650 12.7105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255456_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255456_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255459_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255459_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:44:26.84 -21:10:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.683 5715212963893542016 116.11146652509 -21.16787581170 13.2620 12.2148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255460_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255460_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:05:39.30 -30:27:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.828 5596585726666676736 121.41452869099 -30.45892541213 12.5568 11.8758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255461_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255461_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:07:10.68 -28:52:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.554 5609369713993176320 106.79480023120 -28.87171311362 13.5180 13.0362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255462_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255462_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:07:19.60 -29:23:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.229 5596796558022509440 121.83266832140 -29.39512576071 12.6489 12.1903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255465_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255465_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:22:14.36 -27:49:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.456 5612707655201339392 110.55944658421 -27.81866000870 12.7495 11.7483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255469_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255469_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:46:03.35 -26:39:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.218 5601855411020855680 116.51375682789 -26.65607485001 13.6302 13.2520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255470_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255470_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:31:35.65 -24:11:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.664 5618276720259146368 112.89820108848 -24.19656433722 13.4894 13.1016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255478_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255478_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:10:36.20 -30:27:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.109 5606141444776524416 107.65104156272 -30.45641708805 13.1180 12.4538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255482_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255482_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:14:00.19 -29:54:30.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)
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Considering the candidate 255487_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255487_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:09:02.23 -29:55:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 5.066 5596615310402007936 122.25803649559 -29.91864246419 12.4769 11.9689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255489_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255489_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:15:02.83 -30:49:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.364 5605894084720398336 108.76203830982 -30.83210056551 13.2139 12.5505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255490_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255490_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:13:43.38 -28:29:53.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 255491_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255491_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:39:08.53 -22:49:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.598 5615935963081540096 114.78540777301 -22.82130545239 13.3650 12.8473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255492_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255492_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:56:46.86 -25:10:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.447 5698277976573364992 119.19423395736 -25.17007274018 13.0564 12.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255493_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255493_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 255494_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255494_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:58:38.19 -23:26:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.497 5698737606788829696 119.65894376001 -23.44054795350 13.1183 12.7337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255499_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255499_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:02:15.47 -30:28:27.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)
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Considering the candidate 255501_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255501_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:04:30.76 -28:10:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.204 5597850680433072256 121.12857340258 -28.18137982909 12.8575 12.4369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255502_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255502_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:08:17.27 -28:37:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 0.958 5609465715105236992 107.07194294715 -28.61748811595 13.0662 12.5432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255503_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255503_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:56:37.84 -21:02:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.528 5712405704548731008 119.15740248746 -21.04931784781 13.2478 12.5436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255505_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255505_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:01:38.90 -22:56:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.022 5699145216363193728 120.41152207493 -22.94371997090 13.0702 12.7430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255506_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255506_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 255508_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255508_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255510_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255510_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:11:12.20 -28:45:34.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)
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Considering the candidate 255525_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255525_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:10:26.14 -29:42:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 3.151 5596718797624414976 122.60812709311 -29.70215510114 12.0714 11.3804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255529_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255529_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:09:15.72 -29:16:56.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)
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Considering the candidate 255531_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255531_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:14:21.41 -27:13:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.659 5693867388754337024 123.58844321334 -27.22675966467 12.1950 11.5341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255532_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255532_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255536_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255536_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255537_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255537_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:08:54.27 -22:01:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.032 2928280944054263680 107.22553896208 -22.01890331222 12.6511 11.9208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255539_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255539_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 255540_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255540_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 255541_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255541_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:11:23.29 -29:58:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.151 5606193770354716416 107.84734475106 -29.97371045435 12.7248 12.0482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255543_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255543_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:14:55.15 -28:15:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.001 5692998808925459328 123.72934218653 -28.26064028552 12.0064 11.3128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255546_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255546_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:06:19.76 -30:09:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.036 5607723951244645376 106.58239722840 -30.15883797495 12.6807 12.2957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255550_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255550_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:09:31.58 -30:45:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 2.089 5596319507413081472 122.38099563978 -30.76098029657 11.7963 11.3654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255552_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255552_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255554_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255554_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:02:58.21 -21:11:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.687 5712939551805495680 120.74204034874 -21.19253535353 13.2316 12.5158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255556_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255556_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 255560_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255560_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:09:59.03 -30:18:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 3.529 5596406708118232576 122.49701674966 -30.30542299616 12.0491 11.5634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255561_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255561_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 255563_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255563_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:12:40.04 -30:34:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 5.779 5596428565221567488 123.16501339776 -30.57354373188 11.8915 11.3784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255564_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255564_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:40:00.26 -21:48:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 0.863 5619012942063673984 115.00084666269 -21.81287654173 12.5378 11.7713 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#
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Considering the candidate 255567_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255567_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255568_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255568_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:15:05.94 -26:30:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.820 5694346122991673600 123.77496990600 -26.50272580390 12.0672 11.6169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255569_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255569_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:09:34.54 -29:56:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.970 5596708249184741888 122.39306238207 -29.94697529368 11.9286 11.4917 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255570_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255570_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:15:08.16 -26:57:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 2.933 5694253145536485376 123.78484162940 -26.96301202136 12.1372 11.4487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255571_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255571_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:05:48.49 -30:48:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 3.949 5596189107898709376 121.45098037877 -30.81022123264 12.1073 11.3898 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#
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Considering the candidate 255573_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255573_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:45:53.44 -27:54:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.625 5601437459160142208 116.47226115008 -27.91292038787 12.9512 12.5593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255574_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255574_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 255576_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255576_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:33:12.40 -22:19:07.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)
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Considering the candidate 255583_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255583_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:14:54.69 -30:38:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 4.634 5548399934505484928 123.72637925777 -30.63755601161 11.8563 11.7809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255584_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255584_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:13:46.43 -30:14:47.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)
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Considering the candidate 255586_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255586_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:14:22.08 -30:53:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.461 5548320292941812224 123.59153721148 -30.88547146986 11.6450 10.8581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255588_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255588_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:12:07.83 -25:53:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.713 5611113401999232896 108.03214269961 -25.88298107388 13.3868 12.9357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255589_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255589_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:06:08.89 -29:00:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.524 5609338549710665856 106.53663648213 -29.00903376400 12.5135 11.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255590_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255590_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255591_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255591_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:12:04.63 -30:18:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 5.795 5596452891916019072 123.01775163409 -30.31382440727 11.5473 10.8289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255592_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255592_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:12:05.35 -30:16:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 4.366 5596453750909452160 123.02090485312 -30.28330239074 11.5162 10.8339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255594_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255594_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 255595_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255595_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255598_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255598_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 255602_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255602_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255608_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255608_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:10:04.88 -30:02:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.208 5596516251275397248 122.51941946837 -30.03627118562 11.4599 10.7929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255610_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255610_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255614_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255614_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255616_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255616_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255618_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255618_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 255621_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255621_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255622_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255622_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 255625_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255625_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:45:41.54 -24:47:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.491 5614620053826794880 116.42293964650 -24.78543216119 12.4436 12.3001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255626_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255626_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255627_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255627_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255630_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255630_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255634_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255634_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:14:00.32 -27:38:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 3.965 5693099929638371968 123.50235191023 -27.64464637395 11.5469 10.9334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.965#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255637_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255637_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255640_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255640_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255647_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255647_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255649_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255649_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:13:31.91 -30:21:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.250 5605974834397063424 108.38303783728 -30.36265659195 11.9150 11.1622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255650_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255650_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255651_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255651_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 255652_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255652_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 255653_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255653_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255657_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255657_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:14:50.31 -29:38:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 3.390 5692570686574396032 123.70855906737 -29.63883588507 11.0233 10.4967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255658_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255658_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:54:14.50 -30:27:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 1.437 5595647637084472064 118.56024212806 -30.46221352112 11.7108 11.2550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255659_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255659_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 255660_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255660_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:14:25.83 -29:17:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 2.508 5692632877714437120 123.60734985703 -29.29290398035 11.1437 10.6127 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#
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Considering the candidate 255665_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255665_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:08:05.81 -29:56:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 0.729 5606232047105548160 107.02442470539 -29.94000679961 11.6685 11.3508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255667_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255667_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255668_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255668_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:09:13.77 -21:16:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 4.564 5700960544419000832 122.30825351893 -21.28111517399 11.3434 10.5027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255669_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255669_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 255671_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255671_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:13:33.05 -30:16:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 3.505 5596462650082876800 123.38674076905 -30.26922183967 10.4751 9.8382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255673_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255673_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255674_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255674_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255680_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255680_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 255681_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255681_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:12:17.67 -29:32:45.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)
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Considering the candidate 255682_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255682_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 255686_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255686_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:35:43.97 -23:54:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.93, MAG_FAINT_SEARCH_LIMIT=10.91)GAIADR2_OUTPUT=# 0.837 5615391223791705088 113.93299313769 -23.90667942329 9.7253 8.9297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255688_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255688_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:18:42.34 -24:58:10.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255689_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255689_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:13:57.41 -30:19:34.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255690_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255690_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:44:21.69 -23:53:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.73, MAG_FAINT_SEARCH_LIMIT=11.71)GAIADR2_OUTPUT=# 0.410 5615567248727581568 116.09028513917 -23.88499547447 11.1333 11.0514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255692_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255692_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 255693_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255693_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:44:33.08 -23:50:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 1.753 5615568893688541312 116.13833600027 -23.83945082492 11.4415 11.3804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255696_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255696_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 255697_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255697_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 255698_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255698_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:44:22.03 -23:53:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 1.407 5614816591525382272 116.09177808496 -23.89889067036 11.6791 11.5115 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 255699_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255699_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 255700_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255700_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255702_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255702_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:10:14.02 -27:30:28.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255703_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255703_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:30:44.27 -21:49:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 0.886 5619938391561083520 112.68426394726 -21.82347306324 11.4511 10.5201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255704_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255704_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255705_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255705_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255706_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255706_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:08:09.69 -26:23:58.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255709_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255709_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255710_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255710_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:48:22.29 -25:46:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.360 5602296796222183808 117.09279813478 -25.78320477858 11.2018 9.9873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255711_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255711_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 255713_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255713_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:18:55.21 -26:37:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.053 5616047078172748160 109.72987888979 -26.63086474766 12.0888 11.7795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255714_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255714_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255715_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255715_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255717_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255717_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255718_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255718_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255719_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255719_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 255721_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255721_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255722_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255722_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255723_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255723_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:38:03.43 -25:22:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.800 5614907541752328576 114.51318454036 -25.37230948565 12.4044 11.9030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255725_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255725_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255727_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255727_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:23:55.22 -29:19:05.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255731_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255731_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255735_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255735_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255737_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255737_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255738_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255738_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:35:38.40 -22:51:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.348 5618831973626845696 113.90938772918 -22.85375607051 12.0686 11.0095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255740_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255740_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255741_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255741_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255744_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255744_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255745_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255745_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255747_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255747_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:04:08.23 -27:47:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.418 5597942244829385728 121.03504383180 -27.79017387464 12.2290 10.1112 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255748_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255748_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255749_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255749_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255752_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255752_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255753_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255753_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255754_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255754_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:04:34.04 -29:59:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.803 5596658603673560832 121.14192435898 -29.98808024137 12.1905 11.4223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255755_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255755_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255756_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255756_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:02:36.96 -27:33:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 5.344 5597963174220640128 120.65527151016 -27.56525630463 12.7799 12.0092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255758_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255758_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255759_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255759_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:51:44.65 -21:07:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255761_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255761_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 255762_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255762_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:48:11.74 -25:54:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.489 5602293493379889280 117.04877612847 -25.90946635381 12.6066 12.4327 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#
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Considering the candidate 255764_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255764_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 255766_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255766_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:11:35.31 -20:52:57.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255768_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255768_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255770_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255770_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255771_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255771_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 255772_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255772_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255773_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255773_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:56:20.88 -27:37:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.948 5601082076386485888 119.08649161652 -27.62799408539 12.8174 12.3379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255774_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255774_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 255775_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255775_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255777_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255777_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:27:00.59 -21:37:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.264 5619640320832927744 111.75186925206 -21.62497270771 12.5944 11.6429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255778_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255778_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255780_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255780_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 255781_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255781_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 255783_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255783_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:16:59.31 -21:11:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.735 2929694465028795776 109.24727277159 -21.18940641473 12.8128 12.6165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255784_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255784_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 255785_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255785_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255789_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255789_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:40:42.87 -21:04:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.520 5715194478358037376 115.17877337886 -21.07507037165 12.5312 11.6073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255790_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255790_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255794_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255794_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255795_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255795_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:59:17.24 -24:55:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 2.997 5698297767784272384 119.82097957663 -24.92294449625 12.9495 12.5732 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 255796_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255796_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255797_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255797_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255798_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255798_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255799_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255799_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255801_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255801_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255808_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255808_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255810_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255810_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255812_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255812_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255813_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255813_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:44:03.98 -24:57:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.434 5614607753039133440 116.01553415501 -24.95151280203 12.8271 11.9790 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 255814_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255814_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:49:59.95 -23:46:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.200 5710849723797869824 117.49908763447 -23.77805435386 12.5344 11.5920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255815_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255815_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255816_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255816_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255817_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255817_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255818_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255818_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255819_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255819_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255820_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255820_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255821_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255821_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255824_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255824_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:54:05.35 -26:22:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.506 5601983813362749184 118.52364590987 -26.37108155139 12.9351 12.4962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255826_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255826_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255827_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255827_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255828_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255828_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:42:51.43 -26:19:43.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255829_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255829_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255831_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255831_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255835_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255835_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255836_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255836_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255837_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255837_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:33:52.18 -28:35:14.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
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Considering the candidate 255838_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255838_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255842_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255842_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255843_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255843_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:00:26.59 -26:17:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 0.528 5697356001712735744 120.11089908125 -26.28955503621 13.0260 12.8013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255844_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255844_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 255846_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255846_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:45:03.53 -23:28:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.686 5615607380902972672 116.26430468018 -23.47548133310 12.9807 12.3434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255847_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255847_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:38:47.10 -26:50:04.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255848_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255848_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 255849_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255849_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 255850_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255850_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:55:58.57 -23:00:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.112 5710821583175551488 118.99357131537 -23.00352588154 13.3738 13.1386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255851_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255851_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255853_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255853_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:03:46.87 -29:24:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 5.542 5597445269880289152 120.94695738200 -29.40320816561 11.8192 10.2334 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255854_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255854_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 255855_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255855_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 255856_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255856_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:37:00.30 -21:22:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.502 5619287274521747968 114.25150014366 -21.37334531938 13.2387 12.9329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255857_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255857_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 255858_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255858_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 255859_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255859_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 255865_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255865_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:31:17.86 -28:50:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 5.363 5611698239111252608 112.82353398439 -28.84167118667 13.6052 13.3685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255867_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255867_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:43:38.72 -22:10:19.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 255870_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255870_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:51:11.62 -25:28:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.111 5602409461808277632 117.79793558682 -25.47913377626 13.6783 11.9499 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255873_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255873_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:43:41.38 -28:25:20.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255874_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255874_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 255875_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255875_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:41:10.73 -21:30:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.395 5715101191665224320 115.29412868339 -21.50896799287 13.3142 12.8461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255877_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255877_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 255880_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255880_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:13:54.11 -25:44:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.359 5617123573074688640 108.47678959164 -25.74733478902 13.4904 13.0059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255882_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255882_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255883_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255883_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255885_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255885_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 255887_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255887_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:14:50.00 -27:00:37.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255888_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255888_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255889_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255889_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 255892_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255892_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 255893_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255893_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:52:41.46 -25:32:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.976 5602364240077741824 118.17307146180 -25.54628396471 13.5222 13.2701 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#
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Considering the candidate 255895_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255895_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 255897_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255897_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:48:55.31 -24:57:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.035 5614463304696395392 117.23021560943 -24.95878729416 13.2261 12.6913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255898_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255898_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 255901_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255901_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:42:03.82 -22:01:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 0.939 5712063241041181312 115.51603405345 -22.03193137516 13.5945 13.1538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255905_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255905_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 255909_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255909_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 255910_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255910_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255911_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255911_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:53:05.05 -22:31:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.761 5711094880533742464 118.27029283543 -22.52077549805 13.2377 12.6489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255912_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255912_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 255914_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255914_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:56:21.05 -28:16:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.939 5600485075936743552 119.08766647720 -28.28188053325 13.4558 13.0610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255915_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255915_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 255916_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255916_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 255917_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255917_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 255921_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255921_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 255922_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255922_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 255925_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255925_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:01:48.98 -21:09:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.637 5713106952448586752 120.45427222481 -21.16458587062 13.3472 12.8431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255926_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255926_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 255927_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255927_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:42:52.73 -26:19:52.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255928_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255928_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255929_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255929_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 255930_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255930_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 255931_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255931_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:50:22.64 -25:16:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.584 5602430283809302016 117.59451157820 -25.28287010921 14.0170 13.4556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255934_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255934_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:14:33.60 -24:57:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.009 5617278810374671104 108.63971810292 -24.95478138382 12.9863 12.2939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255935_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255935_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 255936_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255936_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:53:38.54 -22:19:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.336 5711104879217360896 118.41051192376 -22.32622620043 13.7811 13.0082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255937_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255937_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:24:29.49 -27:12:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.934 5613033866552701696 111.12269227297 -27.21520230088 13.2775 12.5958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255938_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255938_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:38:04.51 -25:21:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.211 5614909019221075712 114.51780497504 -25.35655074871 13.6962 13.3335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255940_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255940_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 255941_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255941_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:44:17.63 -21:43:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.357 5712091587826193280 116.07261798580 -21.73076008046 13.3975 12.9531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255944_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255944_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 255945_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255945_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 255948_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255948_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 255949_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255949_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255950_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255950_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:41:10.52 -21:38:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.387 5715095556668189056 115.29479230992 -21.63541180459 13.5752 13.1431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255952_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255952_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:20:06.74 -24:25:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.115 5616936827899691392 110.02751592854 -24.42880766624 13.5127 12.9030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255953_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255953_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 255955_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255955_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 255957_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255957_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 255959_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255959_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:30:44.54 -28:07:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 4.741 5611924910301690624 112.68471017160 -28.13212389204 13.6773 13.2523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255961_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255961_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:03:40.40 -22:27:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.166 5699277123398694784 120.91806343677 -22.45234553015 13.3012 12.8110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255962_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255962_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 255963_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255963_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 255964_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255964_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:50:16.42 -28:29:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.167 5600569016772491904 117.56806547104 -28.49017845652 13.3898 13.0501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255966_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255966_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:05:27.13 -24:03:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 5.717 5698784851426711808 121.36237188826 -24.06193781595 13.7332 13.2594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255968_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255968_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:36:34.44 -26:18:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.223 5612587980226046080 114.14256285123 -26.30055206183 14.3277 13.8374 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255969_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255969_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 255970_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255970_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:07:20.29 -27:20:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.849 5609795706032536704 106.83333824401 -27.33518369897 13.3867 12.5355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255974_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255974_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:57:20.84 -23:01:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.543 5711146901174603264 119.33581804505 -23.01919744628 13.6385 13.1446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255975_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 255975_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 255976_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255976_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255980_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255980_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 255981_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255981_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 255982_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255982_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 255983_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255983_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 255984_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255984_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 255986_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255986_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:19:28.37 -22:01:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.626 5619739517396773376 109.86785160022 -22.02034033619 13.3454 12.9097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255989_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255989_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:02:01.16 -21:42:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.422 5711385460839951744 120.50480458938 -21.70485805303 13.8005 13.0718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255991_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255991_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:07:28.99 -24:32:22.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)
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Considering the candidate 255993_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255993_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:07:57.81 -29:19:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.155 5609291373790429568 106.99025984926 -29.31832163372 13.4770 12.7524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255995_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255995_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 255996_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255996_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255998_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255998_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 255999_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 255999_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 256001_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256001_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:25:28.69 -26:37:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.864 5613088674641898112 111.36844300111 -26.63101607962 13.4921 12.9486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256002_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256002_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 256003_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256003_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:51:48.06 -26:28:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 5.575 5602002814299292032 117.95098028338 -26.47781827678 12.2011 10.7264 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256004_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256004_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:59:46.63 -24:10:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.916 5698639372295500928 119.94371996303 -24.17703314065 14.2666 13.8312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256006_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256006_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:50:01.71 -23:46:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 3.803 5710849758157606400 117.50807670902 -23.77682031642 13.3401 12.2255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256007_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256007_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256008_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256008_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 256012_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256012_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256013_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256013_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 256014_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256014_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 256017_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256017_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 256018_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256018_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256019_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256019_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 256022_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256022_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256023_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256023_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:55:05.18 -21:59:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.208 5711491151394647680 118.77102891021 -21.99794540663 13.8622 13.0318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256025_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256025_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:48:30.02 -22:54:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 4.580 5711726172005047936 117.12380972695 -22.91606304802 13.6702 12.9109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256027_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256027_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:59:59.97 -22:18:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.420 5711291830550452608 119.99945353327 -22.30091371377 13.6419 12.8921 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256028_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256028_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256040_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256040_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256044_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256044_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256048_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256048_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256051_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256051_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256057_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256057_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256058_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256058_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:35:47.32 -22:00:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 2.698 5619038097699324416 113.94676791186 -22.01204093143 13.9048 13.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256066_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256066_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256067_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256067_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256075_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256075_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256079_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256079_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256080_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256080_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:00:02.61 -21:15:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.191 5711613437701976448 120.01075776780 -21.26240418385 13.8965 13.1407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256081_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256081_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256083_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256083_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256084_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256084_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256085_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256085_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256087_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256087_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:45:09.94 -24:19:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.689 5614698119154334720 116.29111242180 -24.32876731707 13.4686 12.6940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256088_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256088_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256089_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256089_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:50:53.39 -24:52:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.940 5614477014233566976 117.72231519995 -24.87978210608 13.8730 13.4467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256093_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256093_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256095_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256095_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:43:43.01 -27:47:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.391 5601638429270660992 115.92877362234 -27.78940799480 14.0440 13.6191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256096_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256096_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256099_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256099_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256100_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256100_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256103_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256103_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 256110_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256110_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256112_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256112_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256118_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256118_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 256119_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256119_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256121_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256121_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:47:59.50 -25:22:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.170 5614343114336515200 116.99761778865 -25.36998645032 13.9708 13.7199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256133_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256133_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256137_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256137_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:48:48.08 -23:47:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 3.231 5614786835990561920 117.19936532062 -23.79003394977 13.7269 12.8033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256138_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256138_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256139_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256139_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 256140_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256140_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 256141_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256141_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:01:22.06 -22:57:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.655 5699144391729565056 120.34130688894 -22.96314477846 14.1826 13.9971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256146_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256146_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:55:26.12 -23:29:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.893 5710735065351011712 118.85860705687 -23.48419140219 13.7561 12.9949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256150_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256150_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:39:45.10 -22:51:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.926 5615920398119987968 114.93764461490 -22.86533385386 14.0635 13.6350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256154_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256154_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 256156_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256156_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:44:34.77 -25:08:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 4.051 5614584216618726784 116.14585123385 -25.13405331588 13.9043 13.0859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256158_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256158_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:39:16.58 -21:30:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.539 5715144313139035904 114.81892795008 -21.51256696840 13.9555 13.3517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256160_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256160_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 256164_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256164_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 256166_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256166_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 256171_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256171_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256175_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256175_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:37:53.98 -28:14:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.576 5600074958095752192 114.47456061290 -28.23336146588 13.7937 12.8654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256177_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256177_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256187_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256187_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:54:15.08 -21:05:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.834 5712416321707870208 118.56290884297 -21.08999850557 14.2429 13.5164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256188_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256188_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:34:16.15 -26:16:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.307 5612599288889993472 113.56688688198 -26.27864300772 14.2343 13.7657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256189_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256189_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256190_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256190_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:48:23.27 -22:39:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.433 5711740087698756352 117.09634050499 -22.66572397482 13.6937 12.7800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256198_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256198_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256200_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256200_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256211_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256211_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256213_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256213_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256218_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256218_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:24:16.84 -22:38:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.499 5619472267352753408 111.06953332059 -22.64502661395 13.7894 12.8476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256232_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 256232_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236079_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 236079_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:09:00.78 -28:00:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.986 5609699120806505216 107.25383714240 -28.00311729013 13.1755 12.3743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237553_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 237553_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:14:23.97 -29:48:26.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 190012_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 190012_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:06:22.53 -22:33:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 5.579 5700714318230850560 121.59553120480 -22.56216708444 11.6290 10.5206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32104_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 32104_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 48019_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 48019_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 28042_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 28042_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 243358_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 243358_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:07:06.30 -30:10:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.538 5604726579468574464 106.77582829532 -30.18308376848 12.0786 11.2608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85109_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 85109_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 13612_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 13612_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 145697_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 145697_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:13:42.24 -24:17:48.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 186098_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 186098_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:59:08.75 -22:26:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46505_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 46505_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 11051_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 11051_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:05:29.78 -30:12:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 2.425 5607702437749429504 106.37485374203 -30.21525910052 12.4452 12.1467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 30020_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 30020_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 212189_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 212189_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 23885_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 23885_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 15143_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 15143_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 95156_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 95156_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 80364_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 80364_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 08511_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 08511_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:09:15.92 -30:39:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 3.067 5596391319269886720 122.31704247329 -30.65820594494 11.8071 10.8938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175035_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 175035_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:10:20.86 -23:00:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24450_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 24450_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 101391_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 101391_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 186264_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 186264_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 57735_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 57735_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 20960_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 20960_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:05:14.97 -29:38:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.02, MAG_FAINT_SEARCH_LIMIT=11.00)GAIADR2_OUTPUT=# 1.542 5607804971507032960 106.31189961980 -29.64172020658 9.8953 9.2244 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#
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Considering the candidate 181203_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 181203_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:15:20.13 -22:00:50.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 08350_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 08350_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 238826_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 238826_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 82462_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 82462_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 04449_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 04449_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 137812_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 137812_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:57:42.50 -24:44:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 4.017 5698317730792004864 119.42821535759 -24.74134391533 10.8325 9.3659 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105656_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 105656_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 238104_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 238104_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:09:20.30 -30:46:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.763 5596319743621255296 122.33408573398 -30.77496117152 12.1167 11.7066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191786_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 191786_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:12:18.79 -22:37:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.502 5700572141934212736 123.07884362792 -22.62080523563 12.9435 12.2752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 172952_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 172952_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 08:09:27.36 -23:06:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.299 5700438035875663744 122.36435121132 -23.11581145804 12.5074 12.0725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 26917_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 26917_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:12:02.67 -29:28:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107348_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 107348_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 237496_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 237496_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:10:37.42 -29:50:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 0.931 5606245344322000000 107.65613665224 -29.84963101209 11.1113 10.6612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236950_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 236950_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:08:10.48 -29:44:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.031 5609243403293724288 107.04320002470 -29.74419069696 12.8863 12.1746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236705_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 236705_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:08:30.08 -23:34:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.894 2927461391268984576 107.12449681530 -23.57359156387 11.8067 10.5182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236228_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 236228_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:12:03.23 -28:36:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.877 5609424174180806784 108.01360707945 -28.60915543075 13.1668 12.4697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 236198_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
The candidate 236198_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007 did not pass the final checks
**** FOUND 07:06:58.66 -28:44:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 0.739 5609559375447985280 106.74433635535 -28.73705384802 12.6049 11.9173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07862_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 07862_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 224372_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 224372_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 61108_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 61108_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 08481_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 08481_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
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Considering the candidate 15371_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
Preparing report for the candidate 15371_fd_Pup-02-Q2b1x1_2026-03-19_20-55-46_20.00sec_-15.00C_LIGHT_0007
make_report_in_HTML.sh Phase 2 (HTML assembly): 15s
make_report_in_HTML.sh TOTAL: 121s
Prepared the HTML report for the field Pup-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:15:30.24 -29:36:52.5
08:14:10.13 -29:36:56.1
07:15:20.11 -22:00:50.1
08:15:12.41 -30:25:31.8
08:13:42.18 -24:17:49.2
07:54:32.25 -23:50:21.0
07:42:27.37 -27:32:06.7
07:21:50.25 -27:56:46.5
07:29:45.37 -29:15:30.9
07:41:33.84 -27:05:29.6
08:15:38.01 -30:49:16.0
07:16:58.03 -30:36:18.7
07:06:12.34 -30:23:31.4
08:13:18.38 -30:36:38.3
08:01:24.42 -25:59:16.1
07:09:33.05 -30:08:53.2
08:14:11.81 -30:14:03.1
07:17:44.55 -30:10:38.4
08:13:09.89 -22:21:16.0
07:19:15.11 -21:07:56.3
08:09:05.97 -21:49:26.8
08:09:47.83 -29:59:22.5
08:07:43.24 -29:47:57.8
07:07:13.76 -29:29:29.7
07:58:25.26 -30:08:48.9
08:04:06.19 -29:08:29.5
08:10:58.84 -30:28:15.6
08:12:25.40 -30:23:54.8
08:13:17.19 -27:45:26.4
08:10:23.15 -30:58:25.2
08:13:20.58 -27:40:23.1
08:11:39.36 -29:21:30.4
08:14:40.35 -28:38:19.2
08:15:39.65 -29:58:15.6
08:15:04.39 -27:15:09.0
08:14:28.76 -30:36:59.2
08:14:58.50 -28:10:07.3
08:13:35.69 -29:35:18.6
08:10:21.54 -30:57:25.8
08:15:25.43 -29:25:43.6
08:14:04.96 -30:11:25.8
08:14:15.44 -30:30:36.4
08:13:52.40 -29:10:34.8
08:12:34.02 -30:39:51.3
08:15:39.82 -29:39:00.5
08:15:07.52 -29:22:49.4
08:15:11.56 -29:39:38.4
08:12:30.88 -20:53:56.0
08:12:38.48 -30:54:27.3
08:15:02.68 -30:30:40.2
07:49:23.64 -26:35:12.6
07:53:21.85 -31:04:52.0
07:42:36.49 -30:47:11.3
08:10:20.65 -29:58:23.2
07:11:44.91 -26:33:29.9
07:05:26.16 -29:16:26.7
07:07:10.58 -29:12:07.9
07:51:29.23 -29:28:21.0
07:07:15.27 -28:23:14.0
07:45:43.92 -28:12:34.3
07:54:36.97 -28:05:00.7
07:29:10.59 -26:53:21.7
07:36:07.93 -26:30:16.5
########### Completed Pup-02-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 ####
08:15:30.24 -29:36:52.5
08:14:10.13 -29:36:56.1
07:15:20.11 -22:00:50.1
08:15:12.41 -30:25:31.8
08:13:42.18 -24:17:49.2
07:54:32.25 -23:50:21.0
07:42:27.37 -27:32:06.7
07:21:50.25 -27:56:46.5
07:29:45.37 -29:15:30.9
07:41:33.84 -27:05:29.6
07:58:25.26 -30:08:48.9
08:04:06.19 -29:08:29.5
08:10:58.84 -30:28:15.6
08:12:25.40 -30:23:54.8
08:13:17.19 -27:45:26.4
08:10:23.15 -30:58:25.2
08:13:20.58 -27:40:23.1
08:11:39.36 -29:21:30.4
08:14:40.35 -28:38:19.2
08:15:39.65 -29:58:15.6
08:15:04.39 -27:15:09.0
08:14:28.76 -30:36:59.2
08:14:58.50 -28:10:07.3
08:13:35.69 -29:35:18.6
08:10:21.54 -30:57:25.8
08:15:25.43 -29:25:43.6
08:14:04.96 -30:11:25.8
08:14:15.44 -30:30:36.4
08:13:52.40 -29:10:34.8
08:12:34.02 -30:39:51.3
08:15:39.82 -29:39:00.5
08:15:07.52 -29:22:49.4
08:15:11.56 -29:39:38.4
08:12:30.88 -20:53:56.0
08:12:38.48 -30:54:27.3
08:15:02.68 -30:30:40.2
07:49:23.64 -26:35:12.6
07:53:21.85 -31:04:52.0
07:42:36.49 -30:47:11.3
08:10:20.65 -29:58:23.2
07:11:44.91 -26:33:29.9
07:51:29.23 -29:28:21.0
07:05:26.16 -29:16:26.7
07:29:10.59 -26:53:21.7
07:09:33.05 -30:08:53.2
07:07:15.27 -28:23:14.0
07:07:10.58 -29:12:07.9
07:19:15.11 -21:07:56.3
08:07:43.24 -29:47:57.8
08:14:11.81 -30:14:03.1
07:36:07.93 -26:30:16.5
07:07:13.76 -29:29:29.7
08:13:09.89 -22:21:16.0
07:45:43.92 -28:12:34.3
07:06:12.34 -30:23:31.4
08:09:47.83 -29:59:22.5
08:15:38.01 -30:49:16.0
08:01:24.42 -25:59:16.1
07:16:58.03 -30:36:18.7
08:09:05.97 -21:49:26.8
07:54:36.97 -28:05:00.7
08:13:18.38 -30:36:38.3
07:17:44.55 -30:10:38.4
###################################################################################
08:15:30.24 -29:36:52.5 -- not an asteroid (will add it to exclusion list)
08:14:10.13 -29:36:56.1 -- not an asteroid (will add it to exclusion list)
07:15:20.11 -22:00:50.1 -- not an asteroid (will add it to exclusion list)
08:15:12.41 -30:25:31.8 -- not an asteroid (will add it to exclusion list)
08:13:42.18 -24:17:49.2 -- not an asteroid (will add it to exclusion list)
07:54:32.25 -23:50:21.0 -- not an asteroid (will add it to exclusion list)
07:42:27.37 -27:32:06.7 -- not an asteroid (will add it to exclusion list)
07:21:50.25 -27:56:46.5 -- not an asteroid (will add it to exclusion list)
07:29:45.37 -29:15:30.9 -- not an asteroid (will add it to exclusion list)
07:41:33.84 -27:05:29.6 -- not an asteroid (will add it to exclusion list)
07:58:25.26 -30:08:48.9 -- not an asteroid (will add it to exclusion list)
08:04:06.19 -29:08:29.5 -- not an asteroid (will add it to exclusion list)
08:10:58.84 -30:28:15.6 -- not an asteroid (will add it to exclusion list)
08:12:25.40 -30:23:54.8 -- not an asteroid (will add it to exclusion list)
08:13:17.19 -27:45:26.4 -- not an asteroid (will add it to exclusion list)
08:10:23.15 -30:58:25.2 -- not an asteroid (will add it to exclusion list)
08:13:20.58 -27:40:23.1 -- not an asteroid (will add it to exclusion list)
08:11:39.36 -29:21:30.4 -- not an asteroid (will add it to exclusion list)
08:14:40.35 -28:38:19.2 -- not an asteroid (will add it to exclusion list)
08:15:39.65 -29:58:15.6 -- not an asteroid (will add it to exclusion list)
08:15:04.39 -27:15:09.0 -- not an asteroid (will add it to exclusion list)
08:14:28.76 -30:36:59.2 -- not an asteroid (will add it to exclusion list)
08:14:58.50 -28:10:07.3 -- not an asteroid (will add it to exclusion list)
08:13:35.69 -29:35:18.6 -- not an asteroid (will add it to exclusion list)
08:10:21.54 -30:57:25.8 -- not an asteroid (will add it to exclusion list)
08:15:25.43 -29:25:43.6 -- not an asteroid (will add it to exclusion list)
08:14:04.96 -30:11:25.8 -- not an asteroid (will add it to exclusion list)
08:14:15.44 -30:30:36.4 -- not an asteroid (will add it to exclusion list)
08:13:52.40 -29:10:34.8 -- not an asteroid (will add it to exclusion list)
08:12:34.02 -30:39:51.3 -- not an asteroid (will add it to exclusion list)
08:15:39.82 -29:39:00.5 -- not an asteroid (will add it to exclusion list)
08:15:07.52 -29:22:49.4 -- not an asteroid (will add it to exclusion list)
08:15:11.56 -29:39:38.4 -- not an asteroid (will add it to exclusion list)
08:12:30.88 -20:53:56.0 -- not an asteroid (will add it to exclusion list)
08:12:38.48 -30:54:27.3 -- not an asteroid (will add it to exclusion list)
08:15:02.68 -30:30:40.2 -- not an asteroid (will add it to exclusion list)
07:49:23.64 -26:35:12.6 -- not an asteroid (will add it to exclusion list)
07:53:21.85 -31:04:52.0 -- not an asteroid (will add it to exclusion list)
07:42:36.49 -30:47:11.3 -- not an asteroid (will add it to exclusion list)
08:10:20.65 -29:58:23.2 -- not an asteroid (will add it to exclusion list)
07:11:44.91 -26:33:29.9 -- not an asteroid (will add it to exclusion list)
07:51:29.23 -29:28:21.0 -- not an asteroid (will add it to exclusion list)
07:05:26.16 -29:16:26.7 -- not an asteroid (will add it to exclusion list)
07:29:10.59 -26:53:21.7 -- not an asteroid (will add it to exclusion list)
07:09:33.05 -30:08:53.2 -- not an asteroid (will add it to exclusion list)
07:07:15.27 -28:23:14.0 -- not an asteroid (will add it to exclusion list)
07:07:10.58 -29:12:07.9 -- not an asteroid (will add it to exclusion list)
07:19:15.11 -21:07:56.3 -- not an asteroid (will add it to exclusion list)
08:07:43.24 -29:47:57.8 -- not an asteroid (will add it to exclusion list)
08:14:11.81 -30:14:03.1 -- not an asteroid (will add it to exclusion list)
07:36:07.93 -26:30:16.5 -- not an asteroid (will add it to exclusion list)
07:07:13.76 -29:29:29.7 -- not an asteroid (will add it to exclusion list)
08:13:09.89 -22:21:16.0 -- not an asteroid (will add it to exclusion list)
07:45:43.92 -28:12:34.3 -- not an asteroid (will add it to exclusion list)
07:06:12.34 -30:23:31.4 -- not an asteroid (will add it to exclusion list)
08:09:47.83 -29:59:22.5 -- not an asteroid (will add it to exclusion list)
08:15:38.01 -30:49:16.0 -- not an asteroid (will add it to exclusion list)
08:01:24.42 -25:59:16.1 -- not an asteroid (will add it to exclusion list)
07:16:58.03 -30:36:18.7 -- not an asteroid (will add it to exclusion list)
08:09:05.97 -21:49:26.8 -- not an asteroid (will add it to exclusion list)
07:54:36.97 -28:05:00.7 -- not an asteroid (will add it to exclusion list)
08:13:18.38 -30:36:38.3 -- not an asteroid (will add it to exclusion list)
07:17:44.55 -30:10:38.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
07:05:26.16 -29:16:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:12.34 -30:23:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:10.58 -29:12:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:13.76 -29:29:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:15.27 -28:23:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:33.05 -30:08:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:44.91 -26:33:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:20.11 -22:00:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:58.03 -30:36:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:44.55 -30:10:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:15.11 -21:07:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:50.25 -27:56:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:29:10.59 -26:53:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:29:45.37 -29:15:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:07.93 -26:30:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:33.84 -27:05:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:27.37 -27:32:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:36.49 -30:47:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:43.92 -28:12:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:49:23.64 -26:35:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:51:29.23 -29:28:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:53:21.85 -31:04:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:54:32.25 -23:50:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:54:36.97 -28:05:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:58:25.26 -30:08:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:01:24.42 -25:59:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:04:06.19 -29:08:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:07:43.24 -29:47:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:09:05.97 -21:49:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:09:47.83 -29:59:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:10:20.65 -29:58:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:10:21.54 -30:57:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:10:23.15 -30:58:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:10:58.84 -30:28:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:39.36 -29:21:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:12:25.40 -30:23:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:12:30.88 -20:53:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:12:34.02 -30:39:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:12:38.48 -30:54:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:09.89 -22:21:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:17.19 -27:45:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:18.38 -30:36:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:20.58 -27:40:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:35.69 -29:35:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:42.18 -24:17:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:52.40 -29:10:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:04.96 -30:11:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:10.13 -29:36:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:11.81 -30:14:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:15.44 -30:30:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:28.76 -30:36:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:40.35 -28:38:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:58.50 -28:10:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:02.68 -30:30:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:04.39 -27:15:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:07.52 -29:22:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:11.56 -29:39:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:12.41 -30:25:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:25.43 -29:25:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:30.24 -29:36:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:38.01 -30:49:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:39.65 -29:58:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:39.82 -29:39:00.5 -- 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)
07:05:26.16 -29:16:26.7 -- not a known variable star
07:06:12.34 -30:23:31.4 -- not a known variable star
07:07:10.58 -29:12:07.9 -- a known variable star
07:07:13.76 -29:29:29.7 -- not a known variable star
07:07:15.27 -28:23:14.0 -- not a known variable star
07:09:33.05 -30:08:53.2 -- not a known variable star
07:11:44.91 -26:33:29.9 -- a known variable star
07:15:20.11 -22:00:50.1 -- a known variable star
07:16:58.03 -30:36:18.7 -- not a known variable star
07:17:44.55 -30:10:38.4 -- a known variable star
07:19:15.11 -21:07:56.3 -- a known variable star
07:21:50.25 -27:56:46.5 -- not a known variable star
07:29:10.59 -26:53:21.7 -- a known variable star
07:29:45.37 -29:15:30.9 -- not a known variable star
07:36:07.93 -26:30:16.5 -- a known variable star
07:41:33.84 -27:05:29.6 -- not a known variable star
07:42:27.37 -27:32:06.7 -- not a known variable star
07:42:36.49 -30:47:11.3 -- a known variable star
07:45:43.92 -28:12:34.3 -- a known variable star
07:49:23.64 -26:35:12.6 -- not a known variable star
07:51:29.23 -29:28:21.0 -- a known variable star
07:53:21.85 -31:04:52.0 -- a known variable star
07:54:32.25 -23:50:21.0 -- a known variable star
07:54:36.97 -28:05:00.7 -- a known variable star
07:58:25.26 -30:08:48.9 -- a known variable star
08:01:24.42 -25:59:16.1 -- a known variable star
08:04:06.19 -29:08:29.5 -- not a known variable star
08:07:43.24 -29:47:57.8 -- a known variable star
08:09:05.97 -21:49:26.8 -- a known variable star
08:09:47.83 -29:59:22.5 -- not a known variable star
08:10:20.65 -29:58:23.2 -- a known variable star
08:10:21.54 -30:57:25.8 -- not a known variable star
08:10:23.15 -30:58:25.2 -- not a known variable star
08:10:58.84 -30:28:15.6 -- not a known variable star
08:11:39.36 -29:21:30.4 -- not a known variable star
08:12:25.40 -30:23:54.8 -- not a known variable star
08:12:30.88 -20:53:56.0 -- not a known variable star
08:12:34.02 -30:39:51.3 -- not a known variable star
08:12:38.48 -30:54:27.3 -- a known variable star
08:13:09.89 -22:21:16.0 -- not a known variable star
08:13:17.19 -27:45:26.4 -- not a known variable star
08:13:18.38 -30:36:38.3 -- not a known variable star
08:13:20.58 -27:40:23.1 -- not a known variable star
08:13:35.69 -29:35:18.6 -- not a known variable star
08:13:42.18 -24:17:49.2 -- a known variable star
08:13:52.40 -29:10:34.8 -- not a known variable star
08:14:04.96 -30:11:25.8 -- not a known variable star
08:14:10.13 -29:36:56.1 -- not a known variable star
08:14:11.81 -30:14:03.1 -- not a known variable star
08:14:15.44 -30:30:36.4 -- not a known variable star
08:14:28.76 -30:36:59.2 -- not a known variable star
08:14:40.35 -28:38:19.2 -- a known variable star
08:14:58.50 -28:10:07.3 -- a known variable star
08:15:02.68 -30:30:40.2 -- not a known variable star
08:15:04.39 -27:15:09.0 -- not a known variable star
08:15:07.52 -29:22:49.4 -- not a known variable star
08:15:11.56 -29:39:38.4 -- not a known variable star
08:15:12.41 -30:25:31.8 -- a known variable star
08:15:25.43 -29:25:43.6 -- not a known variable star
08:15:30.24 -29:36:52.5 -- not a known variable star
08:15:38.01 -30:49:16.0 -- not a known variable star
08:15:39.65 -29:58:15.6 -- not a known variable star
08:15:39.82 -29:39:00.5 -- not a known variable star
Found 40 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
63 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 63 (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)2461119.58002206 -observatory 500
22:37:26.83 -07:25:48.1 Mercury (1.2mag)
01:02:23.45 +05:41:07.4 Venus (-3.9mag)
23:00:28.77 -07:31:08.1 Mars (1.2mag)
07:04:38.52 +22:58:09.2 Jupiter (-2.3mag)
00:16:55.68 -00:28:53.9 Saturn (0.9mag)
03:42:47.86 +19:31:24.7 Uranus (5.8mag)
00:07:09.71 -00:38:51.8 Neptune (7.8mag)
20:31:55.36 -22:53:55.3 Pluto (14.5mag)
00:41:22.90 +07:38:10.7 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Mar 19 22:09 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461119.58002206:
07:04:29.52 +22:58:25.6 Io (5.6mag)
07:04:41.71 +22:57:59.5 Europa (5.7mag)
07:04:29.33 +22:58:18.7 Ganymede (5.2mag)
07:04:10.14 +22:58:53.4 Callisto (6.4mag)
07:08:39.96 +23:00:18.4 Himalia (15.2mag)
07:04:37.91 +22:58:07.4 Thebe (16.0mag)
07:08:13.71 +23:23:10.4 Elara (17.1mag)
07:01:42.96 +23:52:19.5 Pasiphae (17.2mag)
07:13:26.69 +22:52:26.4 Carme (18.3mag)
00:16:47.43 -00:28:42.8 Titan (8.8mag)
00:16:54.79 -00:28:48.3 Rhea (10.1mag)
00:17:26.11 -00:26:55.5 Iapetus (11.5mag)
00:17:09.74 -00:29:02.4 Hyperion (14.8mag)
00:18:50.29 -00:17:33.3 Phoebe (16.8mag)
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461119.58002206:
12:42:09.13 +09:49:29.4 JWST
19:18:14.09 +13:23:25.5 Chandra
15:17:31.45 -59:52:15.9 XMM-Newton
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461119.58002206 -observatory 500
18:34:37.58 -27:25:16.3 14.1mag P/2010 H2 (Vales)
04:50:44.41 -71:05:09.7 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:40.80 +31:17:40.9 17.0mag C/2017 K2 (PANSTARRS)
17:29:28.86 +07:17:40.2 17.6mag C/2021 G2 (ATLAS)
23:01:11.85 +28:25:07.0 16.9mag C/2022 E2 (ATLAS)
03:59:32.79 +25:16:03.9 15.7mag C/2022 N2 (PANSTARRS)
09:01:58.91 +31:24:43.1 16.0mag C/2022 QE78 (ATLAS)
08:30:16.66 -03:17:31.3 17.2mag C/2022 R6 (PANSTARRS)
18:56:28.23 +16:12:46.6 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:26.75 -11:51:13.8 17.6mag P/2023 B1 (PANSTARRS)
09:25:18.31 -16:29:24.6 17.4mag C/2023 F3 (ATLAS)
21:20:18.84 +61:39:59.8 17.4mag C/2023 H5 (Lemmon)
19:33:25.68 -03:31:03.6 14.5mag C/2023 R1 (PANSTARRS)
21:35:33.63 +82:46:20.2 17.7mag C/2023 X2 (Lemmon)
06:15:43.04 +63:47:54.6 16.8mag C/2024 A1 (ATLAS)
04:03:25.32 +04:30:36.5 9.0mag C/2024 E1 (Wierzchos)
11:23:24.09 +02:32:54.3 18.0mag C/2024 G2 (ATLAS)
16:32:35.40 +02:01:14.3 17.5mag C/2024 G6 (ATLAS)
20:09:33.98 +08:33:18.0 14.9mag C/2024 J3 (ATLAS)
03:04:00.50 -26:48:54.3 16.5mag C/2024 T5 (ATLAS)
04:57:00.33 +52:54:01.4 17.6mag C/2025 J1 (Borisov)
15:16:13.74 +16:13:24.8 14.4mag C/2025 L1 (ATLAS)
02:47:23.01 -22:27:39.6 17.6mag C/2025 Q3 (ATLAS)
22:32:19.45 +18:57:07.1 12.6mag C/2025 R3 (PANSTARRS)
13:05:24.92 +01:15:03.7 17.7mag C/2025 Y1 (ATLAS)
02:12:01.76 -06:54:45.6 14.3mag C/2026 A1 (MAPS)
22:35:48.60 +30:45:51.5 13.7mag C/2026 B2 (Sun-Gao)
17:50:16.39 -10:52:01.5 13.4mag 10P/Tempel
15:27:12.92 +05:11:01.0 11.7mag 24P/Schaumasse
11:12:23.13 -02:30:59.5 15.6mag 29P/Schwassmann-Wachmann
17:42:42.54 -10:40:49.0 17.3mag 40P/Vaisala
10:45:38.38 -06:39:39.0 16.4mag 43P/Wolf-Harrington
01:07:34.50 +12:45:26.7 17.0mag 47P/Ashbrook-Jackson
06:27:21.72 +42:31:53.2 17.1mag 63P/Wild
22:52:54.29 -14:51:49.2 15.7mag 65P/Gunn
02:56:20.27 +10:56:18.8 15.9mag 76P/West-Kohoutek-Ikemura
00:07:34.88 +02:51:55.5 14.7mag 78P/Gehrels
21:35:33.77 -16:58:46.5 14.5mag 88P/Howell
00:58:26.37 +12:57:08.4 15.3mag 93P/Lovas
04:09:13.67 +30:37:25.1 16.5mag 123P/West-Hartley
08:07:33.07 +50:40:29.3 16.2mag 124P/Mrkos
01:53:00.86 +11:14:40.6 16.4mag 128P/Shoemaker-Holt
01:55:39.63 +10:54:05.7 17.4mag 131P/Mueller
23:16:04.37 +02:43:52.7 13.1mag 141P/Machholz
23:26:08.31 -04:43:26.7 13.1mag 141P-A/Machholz
22:27:29.23 -07:12:12.8 16.2mag 141P-D/Machholz
23:47:51.30 -14:34:12.0 15.5mag 162P/SidingSpring
10:40:00.06 +32:02:14.7 17.5mag 164P/Christensen
05:48:09.33 +24:44:28.8 17.5mag 198P/ODAS
15:34:30.63 -03:30:00.5 16.9mag 210P/Christensen
20:08:17.65 -17:44:28.3 17.1mag 218P/LINEAR
16:58:17.23 -16:45:14.4 16.3mag 235P/LINEAR
04:39:42.15 +31:52:38.6 16.3mag 240P/NEAT
07:29:44.75 -08:29:56.7 17.5mag 242P/Spahr
15:48:37.01 +05:02:08.7 17.7mag 391P/Kowalski
07:27:55.36 +21:05:29.8 17.5mag 450P/LONEOS
04:59:51.34 +46:40:39.3 17.9mag 493P/LONEOS
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
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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 22:09 tocp_transients_list.txt