This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 962024334449432448,2461128.6479,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962024334449432448 20260329.1479 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:57.03 +44:07:48.5 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_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 197083787085249024,2461128.6479,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197083787085249024 20260329.1479 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:11.25 +44:18:00.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.30 06:11:48.31 +45:45:47.4
167.71767 12.70085 galactic Aur Second-epoch detections are separated by 2.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:11:48.31 +45:45:47.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.560+/-0.035 (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
target,2461128.6479,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1479 13.30CV 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:48.31 +45:45:47.4 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.18 06:18:46.64 +43:56:45.1
169.94654 13.02839 galactic Aur Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J094.6945+43.9433 | 06:18:46.64 +43:56:45.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.482+/-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 J094.6945+43.9433,2461128.6479,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.6945+43.9433 20260329.1479 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:46.64 +43:56:45.1 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.88 06:12:16.01 +42:21:07.8
170.88120 11.26352 galactic Aur Second-epoch detections are separated by 1.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J093.0667+42.3522 | 06:12:16.01 +42:21:07.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.695+/-0.028 (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 J093.0667+42.3522,2461128.6479,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J093.0667+42.3522 20260329.1479 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:16.01 +42:21:07.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.87 06:33:54.47 +44:04:53.0
170.96460 15.56698 galactic Aur Second-epoch detections are separated by 2.2" 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 964937937183849856 | 06:33:53.48 +44:04:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.369+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 964937937183849856,2461128.6479,12.87,0.05,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
Gaia DR3 964937937183849856 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:33:54.47 +44:04:53.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.73 06:21:31.87 +41:49:30.6
172.13388 12.57863 galactic Aur Second-epoch detections are separated by 3.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.3673+41.8196 | 06:21:31.87 +41:49:30.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.672+/-0.029 (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 J095.3673+41.8196,2461128.6479,12.73,0.05,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 J095.3673+41.8196 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:31.87 +41:49:30.6 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.46 05:50:10.12 +43:38:48.8
167.78700 8.31429 galactic Aur Second-epoch detections are separated by 0.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J087.5437+43.6538 | 05:50:09.01 +43:38:31.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.372+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J087.5437+43.6538,2461128.6479,12.46,0.05,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
ATO J087.5437+43.6538 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:10.12 +43:38:48.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.53 05:33:25.76 +42:22:23.4
167.28576 5.03779 galactic Aur Second-epoch detections are separated by 1.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 194668366197812096 | 05:33:28.08 +42:22:29.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.309+/-0.035 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194668366197812096,2461128.6479,12.53,0.05,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 194668366197812096 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:25.76 +42:22:23.4 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 11.47 05:50:23.51 +41:49:03.9
169.40802 7.43729 galactic Aur Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 192332281946145280 | 05:50:23.56 +41:49:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7IV (LAMOST DR5) J-Ks=0.149+/-0.030 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192332281946145280,2461128.6479,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192332281946145280 20260329.1479 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:23.51 +41:49:03.9 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 11.31 05:39:19.54 +42:40:25.7
167.61082 6.11759 galactic Aur Second-epoch detections are separated by 0.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 195993449507080704 | 05:39:19.54 +42:40:25.7 (user input) | 2021A&A...648A..44M | | (position from user input) (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) J-Ks=0.198+/-0.031 (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
Large-amplitude variable Gaia DR2 195993449507080704,2461128.6479,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 195993449507080704 20260329.1479 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:19.54 +42:40:25.7 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 11.57 05:48:33.26 +41:48:56.8
169.23634 7.14028 galactic Aur Second-epoch detections are separated by 0.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 192716728762870272 | 05:48:32.78 +41:49:30.0 (Gaia DR3) | L (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.447+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 192716728762870272,2461128.6479,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192716728762870272 20260329.1479 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:33.26 +41:48:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 11.82 06:02:54.44 +43:29:35.5
169.05090 10.26143 galactic Aur Second-epoch detections are separated by 0.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.7252+43.4870 | 06:02:54.44 +43:29:35.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.275+/-0.030 (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 J090.7252+43.4870,2461128.6479,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.7252+43.4870 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:54.44 +43:29:35.5 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 11.94 06:18:24.35 +42:21:35.0
171.38435 12.28513 galactic Aur Second-epoch detections are separated by 1.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:18:24.35 +42:21:35.0 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6479,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1479 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:24.35 +42:21:35.0 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 11.93 06:21:48.29 +46:46:31.4
167.52840 14.69499 galactic Aur Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.4512+46.7771 | 06:21:48.29 +46:46:31.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J095.4512+46.7771,2461128.6479,11.93,0.05,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
ATO J095.4512+46.7771 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:48.29 +46:46:31.4 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.24 05:56:55.49 +45:30:19.9
166.73637 10.27046 galactic Aur Second-epoch detections are separated by 0.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:56:55.49 +45:30:19.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6479,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1479 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:55.49 +45:30:19.9 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.35 06:26:19.96 +41:59:10.4
172.37033 13.45668 galactic Aur Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:26:19.96 +41:59:10.4 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6479,12.35,0.05,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
target 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:19.96 +41:59:10.4 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_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 959072936002864000,2461128.6479,12.32,0.05,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
Gaia DR3 959072936002864000 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:24:52.08 +43:32:25.0 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.48 06:03:23.01 +42:40:13.5
169.83101 9.95369 galactic Aur Second-epoch detections are separated by 2.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 960874520165473536 | 06:03:21.49 +42:39:52.5 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE J-Ks=0.361+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 960874520165473536,2461128.6479,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 960874520165473536 20260329.1479 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:23.01 +42:40:13.5 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.34 05:29:04.65 +42:17:35.5
166.91382 4.31960 galactic Aur Second-epoch detections are separated by 2.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:29:04.65 +42:17:35.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.236+/-0.030 (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
target,2461128.6479,12.34,0.05,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
target 20260329.1479 12.34CV 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:04.65 +42:17:35.5 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.55 05:55:48.15 +42:30:31.4
169.30048 8.65028 galactic Aur Second-epoch detections are separated by 5.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.9474+42.5087 | 05:55:48.15 +42:30:31.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J088.9474+42.5087,2461128.6479,12.55,0.05,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
ATO J088.9474+42.5087 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:48.15 +42:30:31.4 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.51 05:54:26.17 +41:58:45.0
169.64278 8.17100 galactic Aur Second-epoch detections are separated by 1.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 192393648438331136 | 05:54:22.96 +41:58:25.6 (Gaia DR3) | ACV/roAm/ (local) | (local) | Gaia3var=VARIABLE SpType: A1V (LAMOST DR5) J-Ks=0.390+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 192393648438331136,2461128.6479,12.51,0.05,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 192393648438331136 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:26.17 +41:58:45.0 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.53 06:01:40.52 +44:57:47.7
167.62382 10.75227 galactic Aur Second-epoch detections are separated by 2.4" 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 | target | 06:01:40.52 +44:57:47.7 (user input) | T | P | (position from user input) J-Ks=0.346+/-0.029 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6479,12.53,0.05,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
target 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:40.52 +44:57:47.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.48 05:37:40.65 +43:34:44.7
166.67728 6.33830 galactic Aur Second-epoch detections are separated by 2.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J084.4082+43.5753 | 05:37:37.98 +43:34:31.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.483+/-0.034 (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 J084.4082+43.5753,2461128.6479,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.4082+43.5753 20260329.1479 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:40.65 +43:34:44.7 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.64 06:13:22.40 +44:28:31.0
169.02766 12.38457 galactic Aur Second-epoch detections are separated by 0.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 962064466623651200 | 06:13:20.58 +44:28:05.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 962064466623651200,2461128.6479,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962064466623651200 20260329.1479 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:22.40 +44:28:31.0 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.70 06:40:11.21 +49:27:38.2
166.14913 18.55062 galactic Aur Second-epoch detections are separated by 1.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 967138094309568128 | 06:40:14.42 +49:27:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 967138094309568128,2461128.6479,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 967138094309568128 20260329.1479 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:11.21 +49:27:38.2 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.79 06:31:02.06 +44:18:09.2
170.54407 15.17993 galactic Aur Second-epoch detections are separated by 3.3" 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 | target | 06:31:02.06 +44:18:09.2 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6479,12.79,0.05,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
target 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:02.06 +44:18:09.2 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.61 05:48:20.79 +42:41:23.3
168.45567 7.54762 galactic Aur Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 193002326905083264 | 05:48:20.09 +42:41:59.3 (Gaia DR3) | ROT (local) | G (local) | Gaia3var=VARIABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 193002326905083264,2461128.6479,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 193002326905083264 20260329.1479 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:20.79 +42:41:23.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.69 06:20:04.60 +46:38:02.7
167.53538 14.36681 galactic Aur Second-epoch detections are separated by 3.4" 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 | target | 06:20:04.60 +46:38:02.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6479,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260329.1479 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:04.60 +46:38:02.7 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.77 05:58:13.60 +42:51:14.0
169.21236 9.20710 galactic Aur Second-epoch detections are separated by 2.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.5514+42.8423 | 05:58:13.60 +42:51:14.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J089.5514+42.8423,2461128.6479,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.5514+42.8423 20260329.1479 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:13.60 +42:51:14.0 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.59 05:31:40.34 +42:51:26.0
166.70153 5.02780 galactic Aur Second-epoch detections are separated by 1.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J082.9193+42.8568 | 05:31:40.34 +42:51:26.0 (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 J082.9193+42.8568,2461128.6479,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.9193+42.8568 20260329.1479 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:40.34 +42:51:26.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.72 05:59:38.33 +42:04:23.9
170.03273 9.06190 galactic Aur Second-epoch detections are separated by 1.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:59:38.33 +42:04:23.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6479,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1479 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:38.33 +42:04:23.9 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_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,2461128.6479,12.86,0.05,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
target 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:43.50 +44:56:29.6 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.80 05:52:15.57 +44:44:13.7
167.01506 9.17858 galactic Aur Second-epoch detections are separated by 1.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 196601268981151360 | 05:52:12.43 +44:44:42.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 196601268981151360,2461128.6479,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196601268981151360 20260329.1479 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:15.57 +44:44:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.91 06:32:51.38 +42:04:17.3
172.79901 14.59769 galactic Aur Second-epoch detections are separated by 0.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 958710745706118784 | 06:32:52.57 +42:04:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.588+/-0.030 (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
Gaia DR3 958710745706118784,2461128.6479,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 958710745706118784 20260329.1479 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:32:51.38 +42:04:17.3 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.89 06:02:31.89 +48:11:25.0
164.76958 12.36984 galactic Aur Second-epoch detections are separated by 3.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.6351+48.1884 | 06:02:31.89 +48:11:25.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J090.6351+48.1884,2461128.6479,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.6351+48.1884 20260329.1479 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:31.89 +48:11:25.0 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.87 06:01:16.76 +47:35:45.1
165.21197 11.91122 galactic Aur Second-epoch detections are separated by 1.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.3023+47.5982 | 06:01:16.76 +47:35:45.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J090.3023+47.5982,2461128.6479,12.87,0.05,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
ATO J090.3023+47.5982 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:16.76 +47:35:45.1 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.88 06:25:49.08 +48:15:43.8
166.39811 15.91194 galactic Aur Second-epoch detections are separated by 3.5" 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 967525667862574848 | 06:25:52.69 +48:16:02.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.205+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 967525667862574848,2461128.6479,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 967525667862574848 20260329.1479 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:49.08 +48:15:43.8 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.05 05:57:12.19 +42:33:32.2
169.38253 8.90033 galactic Aur Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:57:12.19 +42:33:32.2 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.040 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6479,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1479 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:12.19 +42:33:32.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.87 05:57:45.35 +45:54:52.4
166.44054 10.59249 galactic Aur Second-epoch detections are separated by 2.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:57:45.35 +45:54:52.4 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.029 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6479,12.87,0.05,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
target 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:45.35 +45:54:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.88 05:51:18.88 +43:17:44.8
168.19935 8.32049 galactic Aur Second-epoch detections are separated by 1.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:51:18.88 +43:17:44.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.526+/-0.031 (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
target,2461128.6479,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1479 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:18.88 +43:17:44.8 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 12.90 06:08:15.07 +45:32:12.1
167.64354 12.04373 galactic Aur Second-epoch detections are separated by 2.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.0678+45.5413 | 06:08:15.07 +45:32:12.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.407+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J092.0678+45.5413,2461128.6479,12.90,0.05,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
ATO J092.0678+45.5413 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:15.07 +45:32:12.1 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_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,2461128.6479,12.90,0.05,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
target 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:30.96 +44:57:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.09 06:08:32.65 +42:33:36.4
170.37623 10.74486 galactic Aur Second-epoch detections are separated by 1.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.1360+42.5599 | 06:08:30.13 +42:33:00.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.339+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J092.1360+42.5599,2461128.6479,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.1360+42.5599 20260329.1479 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:32.65 +42:33:36.4 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.05 06:08:14.71 +44:45:48.8
168.34881 11.69534 galactic Aur Second-epoch detections are separated by 2.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.0627+44.7632 | 06:08:14.71 +44:45:48.8 (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 J092.0627+44.7632,2461128.6479,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.0627+44.7632 20260329.1479 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:14.71 +44:45:48.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.20 05:58:21.80 +43:46:38.0
168.40255 9.67079 galactic Aur Second-epoch detections are separated by 2.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 193346787580418944 | 05:58:23.29 +43:45:56.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5) J-Ks=0.348+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 193346787580418944,2461128.6479,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 193346787580418944 20260329.1479 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:21.80 +43:46:38.0 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.05 05:57:11.21 +42:50:25.6
169.13145 9.03354 galactic Aur Second-epoch detections are separated by 1.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:57:11.21 +42:50:25.6 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6479,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1479 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:11.21 +42:50:25.6 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.20 06:07:54.05 +45:58:48.6
167.21003 12.18779 galactic Aur Second-epoch detections are separated by 2.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 963318524057490944 | 06:07:52.35 +45:58:14.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.018+/-0.174 (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 963318524057490944,2461128.6479,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963318524057490944 20260329.1479 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:54.05 +45:58:48.6 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.16 05:38:59.92 +47:35:33.6
163.34816 8.63371 galactic Aur Second-epoch detections are separated by 3.4" 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 J084.7593+47.5882 | 05:39:02.24 +47:35:17.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.535+/-0.035 (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 J084.7593+47.5882,2461128.6479,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.7593+47.5882 20260329.1479 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:59.92 +47:35:33.6 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.27 05:43:13.20 +43:49:15.3
166.99478 7.31942 galactic Aur Second-epoch detections are separated by 1.9" 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 | ATO J085.8054+43.8208 | 05:43:14.72 +43:49:37.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.207+/-0.044 (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 J085.8054+43.8208,2461128.6479,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.8054+43.8208 20260329.1479 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:43:13.20 +43:49:15.3 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1479 2461128.6479 13.34 05:53:04.40 +46:18:47.2
165.68974 10.07114 galactic Aur Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.2615+46.3117 | 05:53:02.57 +46:18:05.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.445+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J088.2615+46.3117,2461128.6479,13.34,0.05,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
ATO J088.2615+46.3117 20260329.1479 13.34CV 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:04.40 +46:18:47.2 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0546556+483237,2461128.6479,11.54,0.05,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
NSVS J0546556+483237 20260329.1479 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:55.64 +48:32:37.8 ;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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20_00sec_-15_00C_LIGHT_0099_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: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461128.64814940 29.03.2026 03:33:10.108 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 18351
Objects passed selection criteria: 18300
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 14998
Average stars matched: 14642 (97.6264 %)
Memory usage VmPeak: 124496 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 28 23:20:20 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: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461128.64814940 29.03.2026 03:33:10.108 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 200
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 152 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): 132795
Objects passed selection criteria: 132518
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 112469
Average stars matched: 108958 (96.8787 %)
Memory usage VmPeak: 1968260 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 28 23:24:34 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.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: 2461128.64762281
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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits'
wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.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 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:02.176 +45:59:47.11
Angular distance between the image centers 0.04 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 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:00.400 +45:59:50.29
Angular distance between the image centers 0.04 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 06:00:02.176 +45:59:47.11
Second-epoch second image center 06:00:00.400 +45:59:50.29
Angular distance between the image centers 0.00522 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.nhfgZoAPhP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.KeYTLLUmLC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits &> /tmp/tmp.7WlKEYpHbG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits &> /tmp/tmp.g6nOTUeTxe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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-2 101 out of 24266 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 23.040760
a=0.000000 b=1.000000 c=23.040760
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.2 pix Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.5 pix fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
2.5 pix fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
Limiting magnitude estimates:
15.4 mag. Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
15.4 mag. Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.6 mag. fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
14.6 mag. fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.nhfgZoAPhP (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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2260, passed=24266
Got 24266 stars (including 21982 good ones) from the SExtractor catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 24266 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 417 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: 5.91"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 5.36"
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 453 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 5.27"
Estimated accuracy of the plate solution: 3.47"
Excluding outliers - 405 stars left (next iteration limit 389)
The image catalog is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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.KeYTLLUmLC (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/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2222, passed=24282
Got 24282 stars (including 22031 good ones) from the SExtractor catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 24282 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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.7WlKEYpHbG (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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=827, passed=13111
Got 13111 stars (including 12274 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 13111 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits -region wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.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.g6nOTUeTxe (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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=822, passed=13117
Got 13117 stars (including 12284 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 13117 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 935 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: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.68"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits -region wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits'
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31282.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31255_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 31255_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:59:43.46 +44:59:09.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31282_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 31282_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:37:22.96 +46:49:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 0.713 209803315551351552 084.34589502799 +46.82176702889 11.3001 10.9865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31333_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 31333_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:14:59.07 +46:47:46.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Aur-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 ####
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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.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 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:02.176 +45:59:47.11
Angular distance between the image centers 0.04 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 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:00.400 +45:59:50.29
Angular distance between the image centers 0.04 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 06:00:02.176 +45:59:47.11
Second-epoch second image center 06:00:00.400 +45:59:50.29
Angular distance between the image centers 0.00522 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.9mfNbjmJSg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.yoRzUpqkRB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits &> /tmp/tmp.lqmaYX2dhK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits &> /tmp/tmp.qGWlrNrovH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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-2 140 out of 170851 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.801794
a=0.000000 b=1.000000 c=21.801794
From vast_summary.log: estimated ref. image limiting mag.: -7.32
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 154 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.0 pix Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.2 pix fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
2.3 pix fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
Limiting magnitude estimates:
14.5 mag. Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
14.5 mag. Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
13.7 mag. fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
13.7 mag. fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.9mfNbjmJSg (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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=20120, passed=170805
Got 170805 stars (including 150422 good ones) from the SExtractor catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 170805 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 406 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: 6.13"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.06"
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 442 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.05"
Estimated accuracy of the plate solution: 4.14"
Excluding outliers - 409 stars left (next iteration limit 387)
The image catalog is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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.yoRzUpqkRB (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/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=20075, passed=170060
Got 170060 stars (including 149712 good ones) from the SExtractor catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 170060 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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.lqmaYX2dhK (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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=7065, passed=92686
Got 92686 stars (including 85522 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 92686 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits -region wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.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.qGWlrNrovH (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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6922, passed=91630
Got 91630 stars (including 84601 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 91630 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits -region wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Saving fully-calibrated image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-32-24_20.00sec_-15.00C_LIGHT_0099.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.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_2026-03-28_CI_Aur-02-Q2b1x1_231535_TTUQ2b1x1_20478_UMJcMyec/wcs_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100.fits
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out193159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193953.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out193145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39411.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 78s
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: 31s
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Considering the candidate 193145_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193145_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193157_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193157_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193159_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193159_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:09:39.28 +43:48:11.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 193164_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193164_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:40:34.17 +46:53:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193165_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193165_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:42:29.77 +44:43:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.508 197245312213914112 085.62462940332 +44.71832749944 13.8957 13.2499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193170_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193170_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193171_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193171_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:45:33.58 +49:18:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.621 211085139950858112 086.39014713160 +49.31161901149 13.8832 13.2792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193175_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193175_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193179_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193179_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:57:52.38 +48:46:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 0.577 210444502629100544 089.46842056173 +48.77710780595 13.7285 13.0185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193192_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193192_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:05:26.97 +42:40:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193201_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193201_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193204_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193204_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193211_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193211_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:28:39.44 +42:43:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 0.209 958799810442205952 097.16440234056 +42.73155528775 13.7438 12.9800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193222_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193222_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193224_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193224_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193227_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193227_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193231_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193231_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:17:15.76 +41:56:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.390 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193236_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193236_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:16:44.08 +44:42:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.370 962379987803965824 094.18319043390 +44.71153534768 13.5579 13.0286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193237_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193237_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:16:36.23 +44:32:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.107 962371397869379840 094.15117384056 +44.54909987079 13.3865 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193242_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193242_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:12:49.27 +42:16:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193245_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193245_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:33:23.20 +42:25:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.002 194672386287186944 083.34616452696 +42.43205755527 13.2370 12.2626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193248_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193248_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:29:14.86 +41:54:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193249_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193249_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:19:25.31 +44:38:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.452 962202214814317312 094.85547961849 +44.64084749790 13.1782 12.5035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193250_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193250_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:42:01.65 +46:28:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.464 209646837008031616 085.50739242992 +46.47416496998 13.1824 12.4695 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#
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Considering the candidate 193251_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193251_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:11:06.06 +41:55:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.019 960956566924526336 092.77506168430 +41.93017064148 13.2400 12.7156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193257_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193257_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:41:57.55 +44:20:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.247 197084989676093184 085.49065431418 +44.34343392020 12.6672 11.5885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193259_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193259_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:20:12.75 +43:38:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.114 961773920675999104 095.05336462401 +43.64875630381 12.9196 12.2182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193262_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193262_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:09:50.26 +42:20:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 1.112 960984226513406592 092.45966093011 +42.33383267719 12.4990 11.6265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193264_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193264_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193265_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193265_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:15:18.26 +42:25:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 0.302 960281368001322240 093.82613499328 +42.42107465710 12.3874 11.6441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193266_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193266_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:57:45.97 +43:34:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193268_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193268_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:43:27.59 +42:19:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.09, MAG_FAINT_SEARCH_LIMIT=11.07)GAIADR2_OUTPUT=# 0.470 193022397288096512 085.86480449930 +42.32350876868 10.9773 10.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193346_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193346_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:59:43.43 +44:59:09.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 193371_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193371_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:37:22.90 +46:49:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.33, MAG_FAINT_SEARCH_LIMIT=11.31)GAIADR2_OUTPUT=# 1.257 209803315551351552 084.34589502799 +46.82176702889 11.3001 10.9865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193506_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193506_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:11:34.55 +48:44:36.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193546_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193546_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193605_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193605_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:45:42.95 +43:37:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193608_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193608_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:19:04.24 +47:21:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 0.720 968930641861363072 094.76769800520 +47.36474567364 12.5150 12.0779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193622_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193622_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193664_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193664_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:37:44.06 +45:09:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193700_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193700_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193707_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193707_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:24:35.79 +41:36:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 1.105 958495589319466880 096.14947870093 +41.60776104186 12.7992 12.0132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193708_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193708_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:15:03.62 +48:49:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.509 969337323724612608 093.76493977175 +48.82277166858 12.8238 12.2993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193721_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193721_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193745_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193745_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:13:46.68 +44:43:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.303 962063465895464192 093.44440342022 +44.72742362945 12.6467 11.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193760_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193760_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:39:07.56 +44:53:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 1.566 197368109622667392 084.78191388712 +44.88670652218 12.6990 11.8738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193767_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193767_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:36:52.22 +44:44:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193772_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193772_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193783_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193783_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:35:56.10 +43:41:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.302 964176314925857024 098.98386586279 +43.68616326775 12.9575 12.4099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193795_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193795_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:05:50.24 +44:39:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193803_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193803_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:40:03.02 +50:02:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193833_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193833_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:42:07.61 +50:04:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.170 214356977317827200 085.53219554945 +50.07566096651 13.0436 12.3953 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 193835_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193835_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:40:51.21 +48:19:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.819 210971134339379200 085.21413495392 +48.32280102290 12.9608 12.3722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193853_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193853_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 193874_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193874_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:03:13.59 +42:56:28.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193876_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193876_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:57:08.49 +49:03:08.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193882_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193882_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193917_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193917_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193925_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193925_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:49:02.50 +49:49:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.262 211485533981987968 087.26034393516 +49.83283336790 13.1234 12.2992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193934_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193934_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193937_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193937_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:49:32.64 +43:42:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.699 196476989808724224 087.38596124422 +43.70900222684 13.0460 12.1905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193938_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193938_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:17:28.79 +45:52:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.112 962555020608754944 094.36996517508 +45.87230854494 13.3178 12.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193942_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193942_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:59:52.76 +44:00:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.511 193367472142815360 089.96999756978 +44.00566216941 13.1290 12.3826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193947_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193947_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 193951_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193951_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:11:01.06 +47:29:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193953_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193953_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:47:16.33 +46:04:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.299 197524141490742528 086.81759006937 +46.07959594163 13.1672 12.3251 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 193983_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193983_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:53:12.08 +45:24:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.567 196872028016249856 088.30074499759 +45.40620224136 13.2360 12.5061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193985_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193985_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:57:46.09 +45:53:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.744 196952562947733504 089.44232599490 +45.88785721699 13.0324 12.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193986_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193986_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:38:38.30 +41:51:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193988_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 193988_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:35:17.77 +42:18:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.160 194489626838375680 083.82385358200 +42.30712602547 13.3433 12.9194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193996_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 193996_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194013_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194013_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:40:42.96 +48:20:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.090 210971336200363648 085.17944784055 +48.33622155749 13.2097 12.6468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194016_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194016_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194025_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194025_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:40:25.99 +48:47:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.670 211054624206428800 085.10792870304 +48.79313041519 13.3541 12.6586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194032_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194032_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194042_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194042_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194045_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194045_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:47:45.18 +50:03:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194048_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194048_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194058_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194058_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:30:57.38 +43:05:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194066_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194066_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:27:50.44 +42:19:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 4.112 195370954129149312 081.96056057116 +42.32939550208 13.3071 12.4499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194071_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194071_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194083_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194083_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:11:49.33 +45:03:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.292 963207786918929408 092.95523434237 +45.05495257659 13.4231 12.7204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194096_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194096_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:17:34.83 +46:23:45.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194115_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194115_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194116_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194116_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194117_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194117_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:38:24.19 +42:59:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194119_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194119_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:56:30.93 +46:14:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 0.782 197751809117411712 089.12908358575 +46.24714326154 13.6175 12.8385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194125_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194125_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:40:14.21 +50:00:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194129_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194129_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194133_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194133_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:01:04.71 +50:00:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194135_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194135_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:26:58.89 +47:46:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 2.832 966013427057234048 096.74626127815 +47.77581955841 13.6162 13.0724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194142_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194142_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194149_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194149_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:08:02.29 +46:40:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.639 963435214026488704 092.00979468381 +46.68289863325 13.5967 13.1319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194172_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194172_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194178_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194178_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:49:44.72 +44:40:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 2.002 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194180_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194180_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194184_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194184_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 194188_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194188_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:43:06.56 +44:51:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.445 197250427518440192 085.77769553460 +44.85885826898 13.2594 12.2721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194191_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194191_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:53:31.11 +44:15:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.003 196520424814484992 088.37994109512 +44.25250419597 13.6666 13.0703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194193_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194193_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:52:03.67 +49:32:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.634 211244191180148352 088.01550768143 +49.54892102579 13.3825 12.6034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194196_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194196_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194200_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194200_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:28:58.83 +43:48:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.700 195751346492911360 082.24536381357 +43.80799508053 13.6166 13.2330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194201_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194201_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:33:56.82 +46:11:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194207_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194207_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:38:22.19 +42:59:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194217_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194217_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:40:28.14 +42:14:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194218_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194218_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194239_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194239_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:00:14.04 +47:43:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 1.641 963734830944569856 090.05878481423 +47.72069134482 13.5637 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194245_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194245_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194255_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194255_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194256_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194256_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:44:48.26 +48:58:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194266_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194266_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:10:01.92 +47:39:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.325 969468887162852736 092.50786637866 +47.65128419673 13.7413 13.1151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194267_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194267_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:31:00.52 +42:54:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194271_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194271_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:25:57.56 +43:06:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.860 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194290_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194290_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194291_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194291_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 194297_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194297_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194300_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194300_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194301_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194301_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:34:13.60 +41:46:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194304_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194304_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:22:30.58 +46:12:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.635 968436170866744448 095.62879686623 +46.20538276046 13.7294 12.9970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194309_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194309_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:36:57.59 +42:25:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194310_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194310_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:52:21.22 +42:50:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194312_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194312_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194323_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194323_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194363_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194363_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:08:05.01 +45:02:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.123 962871027122871040 092.02043346573 +45.03427793519 13.9306 13.3249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.123#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194365_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194365_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194378_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194378_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194381_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194381_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:11:51.79 +45:03:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.212 963207615120236544 092.96583890432 +45.05666831276 14.0648 13.4839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194389_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194389_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:17:33.26 +46:26:45.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194397_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194397_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:42:30.07 +44:44:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194406_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194406_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:02:52.39 +45:42:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.367 963146592224643200 090.71840891408 +45.70231821898 13.6956 12.9106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194408_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194408_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194435_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194435_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 194440_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194440_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194441_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194441_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:13:33.72 +48:03:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.312 969210708089081216 093.39001337563 +48.05522019758 14.0114 13.4390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194447_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194447_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194460_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194460_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194473_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194473_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:57:24.94 +49:14:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.830 210526725482759552 089.35356580650 +49.24269354636 13.7503 12.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194481_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194481_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194502_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194502_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194509_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194509_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 194521_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194521_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:17:15.30 +42:06:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194523_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194523_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:49:25.58 +42:20:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.830 193164474809048320 087.35669110624 +42.33491068620 13.9992 13.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194542_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194542_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194551_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194551_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194554_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194554_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:31:17.78 +46:25:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.766 209027850616719488 082.82299847399 +46.42981585602 13.7731 12.9103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194564_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 194564_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 194594_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194594_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:54:21.49 +42:55:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.463 193251645465407488 088.59009184359 +42.91869191532 14.2168 13.3674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194606_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 194606_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:04:02.04 +42:01:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52500_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 52500_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:59:44.15 +47:37:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102378_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 102378_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:37:57.13 +44:41:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41230_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 41230_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 05:57:24.00 +48:22:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63136_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 63136_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 06:14:59.04 +46:47:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39411_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 39411_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 69909_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100
The candidate 69909_fd_Aur-02-Q2b1x1_2026-03-28_22-33-10_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 9s
make_report_in_HTML.sh TOTAL: 118s
Prepared the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:13:57.03 +44:07:48.5
05:42:11.25 +44:18:00.6
06:11:48.31 +45:45:47.4
06:18:46.64 +43:56:45.1
06:12:16.01 +42:21:07.8
06:33:54.47 +44:04:53.0
06:21:31.87 +41:49:30.6
05:50:10.12 +43:38:48.8
05:33:25.76 +42:22:23.4
05:50:23.51 +41:49:03.9
05:39:19.54 +42:40:25.7
05:48:33.26 +41:48:56.8
06:02:54.44 +43:29:35.5
06:18:24.35 +42:21:35.0
06:21:48.29 +46:46:31.4
05:56:55.49 +45:30:19.9
06:26:19.96 +41:59:10.4
06:24:52.08 +43:32:25.0
06:03:23.01 +42:40:13.5
05:29:04.65 +42:17:35.5
05:55:48.15 +42:30:31.4
05:54:26.17 +41:58:45.0
06:01:40.52 +44:57:47.7
05:37:40.65 +43:34:44.7
06:13:22.40 +44:28:31.0
06:40:11.21 +49:27:38.2
06:31:02.06 +44:18:09.2
05:48:20.79 +42:41:23.3
06:20:04.60 +46:38:02.7
05:58:13.60 +42:51:14.0
05:31:40.34 +42:51:26.0
05:59:38.33 +42:04:23.9
06:00:43.50 +44:56:29.6
05:52:15.57 +44:44:13.7
06:32:51.38 +42:04:17.3
06:02:31.89 +48:11:25.0
06:01:16.76 +47:35:45.1
06:25:49.08 +48:15:43.8
05:57:12.19 +42:33:32.2
05:57:45.35 +45:54:52.4
05:51:18.88 +43:17:44.8
06:08:15.07 +45:32:12.1
06:01:30.96 +44:57:12.8
06:08:32.65 +42:33:36.4
06:08:14.71 +44:45:48.8
05:58:21.80 +43:46:38.0
05:57:11.21 +42:50:25.6
06:07:54.05 +45:58:48.6
05:38:59.92 +47:35:33.6
05:43:13.20 +43:49:15.3
05:53:04.40 +46:18:47.2
05:46:55.64 +48:32:37.8
########### Completed Aur-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 ####
06:13:57.03 +44:07:48.5
05:42:11.25 +44:18:00.6
06:11:48.31 +45:45:47.4
06:18:46.64 +43:56:45.1
06:12:16.01 +42:21:07.8
06:33:54.47 +44:04:53.0
06:21:31.87 +41:49:30.6
05:50:10.12 +43:38:48.8
05:33:25.76 +42:22:23.4
05:50:23.51 +41:49:03.9
05:39:19.54 +42:40:25.7
05:48:33.26 +41:48:56.8
06:02:54.44 +43:29:35.5
06:18:24.35 +42:21:35.0
06:21:48.29 +46:46:31.4
05:56:55.49 +45:30:19.9
06:26:19.96 +41:59:10.4
06:24:52.08 +43:32:25.0
06:03:23.01 +42:40:13.5
05:29:04.65 +42:17:35.5
05:55:48.15 +42:30:31.4
05:54:26.17 +41:58:45.0
06:01:40.52 +44:57:47.7
05:37:40.65 +43:34:44.7
06:13:22.40 +44:28:31.0
06:40:11.21 +49:27:38.2
06:31:02.06 +44:18:09.2
05:48:20.79 +42:41:23.3
06:20:04.60 +46:38:02.7
05:58:13.60 +42:51:14.0
05:31:40.34 +42:51:26.0
05:59:38.33 +42:04:23.9
06:00:43.50 +44:56:29.6
05:52:15.57 +44:44:13.7
06:32:51.38 +42:04:17.3
06:02:31.89 +48:11:25.0
06:01:16.76 +47:35:45.1
06:25:49.08 +48:15:43.8
05:57:12.19 +42:33:32.2
05:57:45.35 +45:54:52.4
05:51:18.88 +43:17:44.8
06:08:15.07 +45:32:12.1
06:01:30.96 +44:57:12.8
06:08:32.65 +42:33:36.4
06:08:14.71 +44:45:48.8
05:58:21.80 +43:46:38.0
05:57:11.21 +42:50:25.6
06:07:54.05 +45:58:48.6
05:38:59.92 +47:35:33.6
05:43:13.20 +43:49:15.3
05:53:04.40 +46:18:47.2
05:46:55.64 +48:32:37.8
###################################################################################
06:13:57.03 +44:07:48.5 -- not an asteroid (will add it to exclusion list)
05:42:11.25 +44:18:00.6 -- not an asteroid (will add it to exclusion list)
06:11:48.31 +45:45:47.4 -- not an asteroid (will add it to exclusion list)
06:18:46.64 +43:56:45.1 -- not an asteroid (will add it to exclusion list)
06:12:16.01 +42:21:07.8 -- not an asteroid (will add it to exclusion list)
06:33:54.47 +44:04:53.0 -- not an asteroid (will add it to exclusion list)
06:21:31.87 +41:49:30.6 -- not an asteroid (will add it to exclusion list)
05:50:10.12 +43:38:48.8 -- not an asteroid (will add it to exclusion list)
05:33:25.76 +42:22:23.4 -- not an asteroid (will add it to exclusion list)
05:50:23.51 +41:49:03.9 -- not an asteroid (will add it to exclusion list)
05:39:19.54 +42:40:25.7 -- not an asteroid (will add it to exclusion list)
05:48:33.26 +41:48:56.8 -- not an asteroid (will add it to exclusion list)
06:02:54.44 +43:29:35.5 -- not an asteroid (will add it to exclusion list)
06:18:24.35 +42:21:35.0 -- not an asteroid (will add it to exclusion list)
06:21:48.29 +46:46:31.4 -- not an asteroid (will add it to exclusion list)
05:56:55.49 +45:30:19.9 -- not an asteroid (will add it to exclusion list)
06:26:19.96 +41:59:10.4 -- not an asteroid (will add it to exclusion list)
06:24:52.08 +43:32:25.0 -- not an asteroid (will add it to exclusion list)
06:03:23.01 +42:40:13.5 -- not an asteroid (will add it to exclusion list)
05:29:04.65 +42:17:35.5 -- not an asteroid (will add it to exclusion list)
05:55:48.15 +42:30:31.4 -- not an asteroid (will add it to exclusion list)
05:54:26.17 +41:58:45.0 -- not an asteroid (will add it to exclusion list)
06:01:40.52 +44:57:47.7 -- not an asteroid (will add it to exclusion list)
05:37:40.65 +43:34:44.7 -- not an asteroid (will add it to exclusion list)
06:13:22.40 +44:28:31.0 -- not an asteroid (will add it to exclusion list)
06:40:11.21 +49:27:38.2 -- not an asteroid (will add it to exclusion list)
06:31:02.06 +44:18:09.2 -- not an asteroid (will add it to exclusion list)
05:48:20.79 +42:41:23.3 -- not an asteroid (will add it to exclusion list)
06:20:04.60 +46:38:02.7 -- not an asteroid (will add it to exclusion list)
05:58:13.60 +42:51:14.0 -- not an asteroid (will add it to exclusion list)
05:31:40.34 +42:51:26.0 -- not an asteroid (will add it to exclusion list)
05:59:38.33 +42:04:23.9 -- not an asteroid (will add it to exclusion list)
06:00:43.50 +44:56:29.6 -- not an asteroid (will add it to exclusion list)
05:52:15.57 +44:44:13.7 -- not an asteroid (will add it to exclusion list)
06:32:51.38 +42:04:17.3 -- not an asteroid (will add it to exclusion list)
06:02:31.89 +48:11:25.0 -- not an asteroid (will add it to exclusion list)
06:01:16.76 +47:35:45.1 -- not an asteroid (will add it to exclusion list)
06:25:49.08 +48:15:43.8 -- not an asteroid (will add it to exclusion list)
05:57:12.19 +42:33:32.2 -- not an asteroid (will add it to exclusion list)
05:57:45.35 +45:54:52.4 -- not an asteroid (will add it to exclusion list)
05:51:18.88 +43:17:44.8 -- not an asteroid (will add it to exclusion list)
06:08:15.07 +45:32:12.1 -- not an asteroid (will add it to exclusion list)
06:01:30.96 +44:57:12.8 -- not an asteroid (will add it to exclusion list)
06:08:32.65 +42:33:36.4 -- not an asteroid (will add it to exclusion list)
06:08:14.71 +44:45:48.8 -- not an asteroid (will add it to exclusion list)
05:58:21.80 +43:46:38.0 -- not an asteroid (will add it to exclusion list)
05:57:11.21 +42:50:25.6 -- not an asteroid (will add it to exclusion list)
06:07:54.05 +45:58:48.6 -- not an asteroid (will add it to exclusion list)
05:38:59.92 +47:35:33.6 -- not an asteroid (will add it to exclusion list)
05:43:13.20 +43:49:15.3 -- not an asteroid (will add it to exclusion list)
05:53:04.40 +46:18:47.2 -- not an asteroid (will add it to exclusion list)
05:46:55.64 +48:32:37.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:29:04.65 +42:17:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:40.34 +42:51:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:25.76 +42:22:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:40.65 +43:34:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:59.92 +47:35:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:19.54 +42:40:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:11.25 +44:18:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:13.20 +43:49:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:55.64 +48:32:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:20.79 +42:41:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:33.26 +41:48:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:10.12 +43:38:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:23.51 +41:49:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.88 +43:17:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:15.57 +44:44:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:04.40 +46:18:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:26.17 +41:58:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:48.15 +42:30:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:55.49 +45:30:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:11.21 +42:50:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:12.19 +42:33:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:45.35 +45:54:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:13.60 +42:51:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:21.80 +43:46:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:38.33 +42:04:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:43.50 +44:56:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:16.76 +47:35:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:30.96 +44:57:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:40.52 +44:57:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:31.89 +48:11:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:54.44 +43:29:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:23.01 +42:40:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:54.05 +45:58:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:14.71 +44:45:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:15.07 +45:32:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:32.65 +42:33:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:48.31 +45:45:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:16.01 +42:21:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:22.40 +44:28:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:57.03 +44:07:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:24.35 +42:21:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:46.64 +43:56:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:04.60 +46:38:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:31.87 +41:49:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:48.29 +46:46:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:52.08 +43:32:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:49.08 +48:15:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.96 +41:59:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:02.06 +44:18:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:51.38 +42:04:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:54.47 +44:04:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:11.21 +49:27:38.2 -- 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)
05:29:04.65 +42:17:35.5 -- not a known variable star
05:31:40.34 +42:51:26.0 -- not a known variable star
05:33:25.76 +42:22:23.4 -- not a known variable star
05:37:40.65 +43:34:44.7 -- not a known variable star
05:38:59.92 +47:35:33.6 -- not a known variable star
05:39:19.54 +42:40:25.7 -- not a known variable star
05:42:11.25 +44:18:00.6 -- a known variable star
05:43:13.20 +43:49:15.3 -- not a known variable star
05:46:55.64 +48:32:37.8 -- a known variable star
05:48:20.79 +42:41:23.3 -- not a known variable star
05:48:33.26 +41:48:56.8 -- not a known variable star
05:50:10.12 +43:38:48.8 -- not a known variable star
05:50:23.51 +41:49:03.9 -- not a known variable star
05:51:18.88 +43:17:44.8 -- not a known variable star
05:52:15.57 +44:44:13.7 -- not a known variable star
05:53:04.40 +46:18:47.2 -- not a known variable star
05:54:26.17 +41:58:45.0 -- not a known variable star
05:55:48.15 +42:30:31.4 -- not a known variable star
05:56:55.49 +45:30:19.9 -- not a known variable star
05:57:11.21 +42:50:25.6 -- not a known variable star
05:57:12.19 +42:33:32.2 -- not a known variable star
05:57:45.35 +45:54:52.4 -- not a known variable star
05:58:13.60 +42:51:14.0 -- not a known variable star
05:58:21.80 +43:46:38.0 -- not a known variable star
05:59:38.33 +42:04:23.9 -- not a known variable star
06:00:43.50 +44:56:29.6 -- not a known variable star
06:01:16.76 +47:35:45.1 -- not a known variable star
06:01:30.96 +44:57:12.8 -- not a known variable star
06:01:40.52 +44:57:47.7 -- not a known variable star
06:02:31.89 +48:11:25.0 -- not a known variable star
06:02:54.44 +43:29:35.5 -- not a known variable star
06:03:23.01 +42:40:13.5 -- not a known variable star
06:07:54.05 +45:58:48.6 -- not a known variable star
06:08:14.71 +44:45:48.8 -- not a known variable star
06:08:15.07 +45:32:12.1 -- not a known variable star
06:08:32.65 +42:33:36.4 -- not a known variable star
06:11:48.31 +45:45:47.4 -- not a known variable star
06:12:16.01 +42:21:07.8 -- not a known variable star
06:13:22.40 +44:28:31.0 -- not a known variable star
06:13:57.03 +44:07:48.5 -- a known variable star
06:18:24.35 +42:21:35.0 -- not a known variable star
06:18:46.64 +43:56:45.1 -- not a known variable star
06:20:04.60 +46:38:02.7 -- not a known variable star
06:21:31.87 +41:49:30.6 -- not a known variable star
06:21:48.29 +46:46:31.4 -- not a known variable star
06:24:52.08 +43:32:25.0 -- a known variable star
06:25:49.08 +48:15:43.8 -- not a known variable star
06:26:19.96 +41:59:10.4 -- not a known variable star
06:31:02.06 +44:18:09.2 -- not a known variable star
06:32:51.38 +42:04:17.3 -- not a known variable star
06:33:54.47 +44:04:53.0 -- not a known variable star
06:40:11.21 +49:27:38.2 -- not a known variable star
Found 48 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
52 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 52 (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)2461128.64762281 -observatory 500
22:51:41.66 -08:08:30.9 Mercury (0.5mag)
01:43:54.99 +10:09:13.1 Venus (-3.9mag)
23:26:48.51 -04:43:33.4 Mars (1.2mag)
07:06:19.67 +22:55:56.4 Jupiter (-2.2mag)
00:21:05.04 -00:02:09.6 Saturn (0.9mag)
03:44:15.41 +19:36:16.8 Uranus (5.8mag)
00:08:25.38 -00:30:44.5 Neptune (7.8mag)
20:32:40.82 -22:52:54.8 Pluto (14.5mag)
09:34:38.85 +16:04:58.8 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Mar 28 23:20 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461128.64762281:
07:06:13.43 +22:56:10.1 Io (5.7mag)
07:06:20.66 +22:55:57.6 Europa (5.8mag)
07:06:01.23 +22:56:35.4 Ganymede (5.2mag)
07:06:52.76 +22:54:58.7 Callisto (6.5mag)
07:10:15.29 +22:52:51.3 Himalia (15.2mag)
07:06:18.31 +22:56:01.4 Thebe (16.1mag)
07:10:01.12 +23:19:20.9 Elara (17.2mag)
07:03:59.93 +23:45:18.7 Pasiphae (17.3mag)
07:14:59.92 +22:51:45.8 Carme (18.4mag)
00:21:13.01 -00:01:55.1 Titan (8.8mag)
00:21:04.27 -00:02:04.8 Rhea (10.1mag)
00:21:23.14 -00:00:00.1 Iapetus (11.5mag)
00:21:00.01 -00:01:43.7 Hyperion (14.8mag)
00:22:54.54 +00:08:25.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 28 23:20 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461128.64762281:
13:53:14.15 -00:00:59.9 JWST
16:28:39.19 +48:04:08.2 Chandra
07:55:53.62 -29:00:43.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 28 23:20 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461128.64762281 -observatory 500
18:41:50.25 -27:50:05.6 14.0mag P/2010 H2 (Vales)
04:55:18.40 -70:34:36.5 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:26.81 +31:20:02.5 17.1mag C/2017 K2 (PANSTARRS)
17:30:37.90 +08:23:30.0 17.6mag C/2021 G2 (ATLAS)
23:04:37.12 +28:37:28.4 17.0mag C/2022 E2 (ATLAS)
04:09:06.78 +25:31:51.9 15.8mag C/2022 N2 (PANSTARRS)
09:01:28.46 +31:43:29.1 16.1mag C/2022 QE78 (ATLAS)
08:29:46.52 -02:10:38.7 17.2mag C/2022 R6 (PANSTARRS)
18:56:22.21 +16:59:45.7 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:13.92 -11:45:41.1 17.6mag P/2023 B1 (PANSTARRS)
09:18:09.97 -14:53:35.5 17.5mag C/2023 F3 (ATLAS)
21:33:16.77 +62:00:06.6 17.4mag C/2023 H5 (Lemmon)
19:30:29.74 -03:33:08.8 14.4mag C/2023 R1 (PANSTARRS)
21:41:44.46 +83:40:10.3 17.8mag C/2023 X2 (Lemmon)
06:13:51.92 +63:40:35.4 16.9mag C/2024 A1 (ATLAS)
04:30:28.84 +10:31:00.6 9.8mag C/2024 E1 (Wierzchos)
16:29:03.69 +03:27:52.7 17.4mag C/2024 G6 (ATLAS)
20:14:07.34 +10:40:49.5 14.8mag C/2024 J3 (ATLAS)
03:11:04.92 -25:15:04.7 16.4mag C/2024 T5 (ATLAS)
05:02:45.92 +50:06:35.3 17.6mag C/2025 J1 (Borisov)
14:48:53.29 +28:12:44.8 14.5mag C/2025 L1 (ATLAS)
02:59:05.50 -23:38:27.2 17.7mag C/2025 Q3 (ATLAS)
22:39:48.11 +19:32:51.1 11.4mag C/2025 R3 (PANSTARRS)
13:01:49.12 +01:51:27.9 17.6mag C/2025 Y1 (ATLAS)
01:44:14.29 -00:56:58.9 11.6mag C/2026 A1 (MAPS)
23:05:41.84 +33:19:09.1 14.0mag C/2026 B2 (Sun-Gao)
18:08:02.34 -10:33:55.4 12.9mag 10P/Tempel
15:21:13.80 +04:40:51.9 12.5mag 24P/Schaumasse
11:08:41.79 -02:09:58.0 15.7mag 29P/Schwassmann-Wachmann
17:51:10.71 -10:19:22.0 17.5mag 40P/Vaisala
10:41:23.99 -05:43:58.9 16.6mag 43P/Wolf-Harrington
01:21:16.43 +14:22:47.2 17.1mag 47P/Ashbrook-Jackson
06:40:18.63 +40:43:18.7 17.1mag 63P/Wild
23:05:29.10 -13:40:44.5 15.7mag 65P/Gunn
03:17:44.45 +14:38:08.8 15.9mag 76P/West-Kohoutek-Ikemura
00:26:46.30 +04:40:36.2 14.5mag 78P/Gehrels
22:06:21.69 -14:33:26.5 14.5mag 88P/Howell
01:21:43.07 +15:37:57.3 15.2mag 93P/Lovas
04:23:19.58 +31:13:20.0 16.4mag 123P/West-Hartley
08:11:33.72 +46:35:16.5 16.2mag 124P/Mrkos
02:06:12.60 +12:19:08.5 16.4mag 128P/Shoemaker-Holt
02:12:54.06 +12:10:26.6 17.4mag 131P/Mueller
23:57:02.21 +06:23:28.2 12.0mag 141P/Machholz
00:07:18.31 -01:42:08.1 12.1mag 141P-A/Machholz
23:02:49.60 -04:48:46.0 15.1mag 141P-D/Machholz
00:12:55.24 -10:19:31.4 15.3mag 162P/SidingSpring
10:34:23.01 +31:52:50.0 17.7mag 164P/Christensen
06:03:56.01 +24:40:03.0 17.7mag 198P/ODAS
15:21:51.31 -02:15:17.3 17.1mag 210P/Christensen
20:41:46.71 -15:43:47.4 17.3mag 218P/LINEAR
17:06:59.30 -15:55:17.0 16.2mag 235P/LINEAR
04:57:16.48 +33:00:15.4 16.5mag 240P/NEAT
07:31:35.90 -07:17:28.9 17.6mag 242P/Spahr
15:47:42.43 +05:42:50.9 17.6mag 391P/Kowalski
07:29:03.74 +21:13:40.6 17.6mag 450P/LONEOS
05:11:08.43 +46:05:59.0 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Mar 28 23:20 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
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
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
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
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
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
18:38:35.79 -79:28:57.30 ASASSN-26bb 2026-02-24.37 16.2
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
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
-rw-r--r-- 1 apache apache 5.8K Mar 28 23:20 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 28 23:20 tocp_transients_list.txt
