This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.91 05:38:47.21 +45:24:51.0
165.20848 7.46991 galactic Aur Second-epoch detections are separated by 2.1" and 6.4 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 J084.7111+45.4051 | 05:38:48.44 +45:24:31.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.208+/-0.032 (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 J084.7111+45.4051,2461129.6506,12.91,0.05,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
ATO J084.7111+45.4051 20260330.1506 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:47.21 +45:24:51.0 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.71 05:53:45.51 +44:06:45.2
167.69944 9.10663 galactic Aur Second-epoch detections are separated by 1.3" and 6.3 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 J088.4375+44.1163 | 05:53:45.51 +44:06:45.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J088.4375+44.1163,2461129.6506,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.4375+44.1163 20260330.1506 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:45.51 +44:06:45.2 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.68 05:35:47.07 +43:12:12.8
166.81415 5.84762 galactic Aur Second-epoch detections are separated by 2.5" and 6.3 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 J083.9393+43.2021 | 05:35:47.07 +43:12:12.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (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 J083.9393+43.2021,2461129.6506,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.9393+43.2021 20260330.1506 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:47.07 +43:12:12.8 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.77 05:29:09.68 +43:57:13.0
165.52908 5.24322 galactic Aur Second-epoch detections are separated by 1.3" and 6.5 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 195761791853371008 | 05:29:11.84 +43:57:09.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 195761791853371008,2461129.6506,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195761791853371008 20260330.1506 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:09.68 +43:57:13.0 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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,2461129.6506,12.46,0.05,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
target 20260330.1506 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:09.07 +44:09:21.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.32 05:30:25.33 +43:26:20.8
166.08681 5.15300 galactic Aur Second-epoch detections are separated by 1.7" and 6.4 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 J082.6110+43.4402 | 05:30:25.33 +43:26:20.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.376+/-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
ATO J082.6110+43.4402,2461129.6506,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.6110+43.4402 20260330.1506 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:25.33 +43:26:20.8 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.20 06:31:06.84 +48:10:19.5
166.83924 16.69110 galactic Aur Second-epoch detections are separated by 2.5" and 5.9 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 967478869899363072 | 06:31:06.85 +48:09:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.347+/-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 967478869899363072,2461129.6506,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 967478869899363072 20260330.1506 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:06.84 +48:10:19.5 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.11 06:19:17.98 +48:31:23.4
165.69988 15.02530 galactic Aur Second-epoch detections are separated by 0.9" and 5.9 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 | 06:19:17.98 +48:31:23.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.316+/-0.028 (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,2461129.6506,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260330.1506 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:17.98 +48:31:23.4 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 11.72 05:38:22.31 +42:05:46.6
168.01123 5.66380 galactic Aur Second-epoch detections are separated by 1.2" and 6.5 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 J084.5993+42.0894 | 05:38:20.62 +42:05:39.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.245+/-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
ATO J084.5993+42.0894,2461129.6506,11.72,0.05,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
ATO J084.5993+42.0894 20260330.1506 11.72CV 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:22.31 +42:05:46.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 11.76 05:41:49.15 +41:45:07.3
168.64378 6.02947 galactic Aur Second-epoch detections are separated by 0.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:41:49.15 +41:45:07.3 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.306+/-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
target,2461129.6506,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260330.1506 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:49.15 +41:45:07.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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 195388992991534720,2461129.6506,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195388992991534720 20260330.1506 11.79CV 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:06.84 +42:29:53.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 11.04 05:57:09.05 +46:13:43.3
166.10851 10.64901 galactic Aur Second-epoch detections are separated by 0.9" and 6.4 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 J089.2879+46.2213 | 05:57:07.32 +46:13:43.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-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
ATO J089.2879+46.2213,2461129.6506,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.2879+46.2213 20260330.1506 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:09.05 +46:13:43.3 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 10.26 05:37:22.95 +46:49:17.9
163.86917 7.99806 galactic Aur Second-epoch detections are separated by 0.3" and 6.3 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 J084.3456+46.8139 | 05:37:26.36 +46:49:16.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.127+/-0.035 (A)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3456+46.8139,2461129.6506,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3456+46.8139 20260330.1506 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:22.95 +46:49:17.9 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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 208040106922999808,2461129.6506,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208040106922999808 20260330.1506 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:26:36.91 +44:48:50.3 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 11.26 05:25:37.67 +45:40:56.8
163.73291 5.67263 galactic Aur Second-epoch detections are separated by 0.5" and 6.6 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 208934456550670592 | 05:25:33.57 +45:41:08.6 (Gaia DR3) | E (local) | A (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.203+/-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
Gaia DR3 208934456550670592,2461129.6506,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208934456550670592 20260330.1506 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:37.67 +45:40:56.8 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 11.23 05:39:19.47 +42:40:25.4
167.61078 6.11736 galactic Aur Second-epoch detections are separated by 0.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 195993449507080704 | 05:39:19.47 +42:40:25.4 (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 195993449507080704,2461129.6506,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 195993449507080704 20260330.1506 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:19.47 +42:40:25.4 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 11.41 05:51:47.60 +48:44:50.8
163.41549 11.05827 galactic Aur Second-epoch detections are separated by 0.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 211144406203922176 | 05:51:50.96 +48:44:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1952CoRut..32....1H BD+48 1314 J-Ks=0.501+/-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
Gaia DR3 211144406203922176,2461129.6506,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211144406203922176 20260330.1506 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:47.60 +48:44:50.8 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 11.81 06:15:03.58 +48:49:21.6
165.11806 14.51233 galactic Aur Second-epoch detections are separated by 1.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J093.7668+48.8348 | 06:15:03.58 +48:49:21.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.371+/-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 J093.7668+48.8348,2461129.6506,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J093.7668+48.8348 20260330.1506 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:03.58 +48:49:21.6 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.00 05:51:18.31 +46:14:40.9
165.59940 9.77097 galactic Aur Second-epoch detections are separated by 2.2" and 6.4 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 J087.7984+46.2495 | 05:51:14.55 +46:14:50.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-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 J087.7984+46.2495,2461129.6506,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.7984+46.2495 20260330.1506 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:18.31 +46:14:40.9 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.03 05:48:04.00 +43:19:51.0
167.87076 7.82606 galactic Aur Second-epoch detections are separated by 3.1" and 6.5 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 J087.0101+43.3293 | 05:48:00.35 +43:19:56.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J087.0101+43.3293,2461129.6506,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J087.0101+43.3293 20260330.1506 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:04.00 +43:19:51.0 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.29 05:43:52.93 +47:06:14.7
164.20148 9.09420 galactic Aur Second-epoch detections are separated by 1.8" and 6.4 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 J085.9886+47.0957 | 05:43:54.70 +47:05:35.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.326+/-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 J085.9886+47.0957,2461129.6506,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.9886+47.0957 20260330.1506 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:43:52.93 +47:06:14.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.19 05:35:42.02 +42:29:11.9
167.41535 5.45232 galactic Aur Second-epoch detections are separated by 1.4" and 6.6 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 | ASASSN-V J053541.13+422836.6 | 05:35:41.14 +42:28:36.6 (Gaia DR3) | SRS (local) | 27.206000000000 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053541.13+422836.6,2461129.6506,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053541.13+422836.6 20260330.1506 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:42.02 +42:29:11.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.21 05:37:23.76 +47:29:29.9
163.29328 8.35013 galactic Aur Second-epoch detections are separated by 1.5" and 6.2 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 J084.3251+47.4864 | 05:37:20.76 +47:29:14.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.413+/-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
ATO J084.3251+47.4864,2461129.6506,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3251+47.4864 20260330.1506 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:23.76 +47:29:29.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.45 06:26:58.99 +47:46:34.8
166.94226 15.90065 galactic Aur Second-epoch detections are separated by 4.3" and 5.6 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 966013392697495936 | 06:26:58.36 +47:45:53.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.410+/-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 966013392697495936,2461129.6506,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 966013392697495936 20260330.1506 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:58.99 +47:46:34.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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 194489626838375680,2461129.6506,12.34,0.05,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
Gaia DR3 194489626838375680 20260330.1506 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:17.67 +42:18:25.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.57 05:26:06.50 +46:10:28.8
163.36722 6.01456 galactic Aur Second-epoch detections are separated by 1.2" and 6.3 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 209147658726555008 | 05:26:02.98 +46:10:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (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 209147658726555008,2461129.6506,12.57,0.05,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 209147658726555008 20260330.1506 12.57CV 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:26:06.50 +46:10:28.8 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.44 05:37:40.49 +43:34:43.9
166.67721 6.33777 galactic Aur Second-epoch detections are separated by 1.4" and 6.6 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 J084.4082+43.5753 | 05:37:37.98 +43:34:31.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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+43.5753,2461129.6506,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.4082+43.5753 20260330.1506 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:40.49 +43:34:43.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.54 05:40:17.40 +46:01:07.2
164.82491 8.00825 galactic Aur Second-epoch detections are separated by 1.8" and 6.6 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 209484933918381952 | 05:40:19.96 +46:00:39.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5) J-Ks=0.436+/-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 209484933918381952,2461129.6506,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 209484933918381952 20260330.1506 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:40:17.40 +46:01:07.2 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.42 05:31:40.31 +42:51:24.2
166.70191 5.02746 galactic Aur Second-epoch detections are separated by 3.1" and 7.2 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 J082.9193+42.8568 | 05:31:40.31 +42:51:24.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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+42.8568,2461129.6506,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.9193+42.8568 20260330.1506 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:40.31 +42:51:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.61 05:28:11.60 +43:27:55.4
165.84231 4.82898 galactic Aur Second-epoch detections are separated by 1.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J082.0489+43.4659 | 05:28:14.53 +43:28:03.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.0489+43.4659,2461129.6506,12.61,0.05,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
ATO J082.0489+43.4659 20260330.1506 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:11.60 +43:27:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.59 05:49:05.93 +45:12:36.2
166.31921 8.92582 galactic Aur Second-epoch detections are separated by 1.4" and 6.5 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 J087.2644+45.2125 | 05:49:03.31 +45:12:21.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A6IV (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 J087.2644+45.2125,2461129.6506,12.59,0.05,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 J087.2644+45.2125 20260330.1506 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:05.93 +45:12:36.2 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.46 05:37:46.19 +43:03:13.0
167.13512 6.07519 galactic Aur Second-epoch detections are separated by 1.6" and 6.4 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 J084.4314+43.0363 | 05:37:45.51 +43:02:45.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.634+/-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
ATO J084.4314+43.0363,2461129.6506,12.46,0.05,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 J084.4314+43.0363 20260330.1506 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:46.19 +43:03:13.0 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.73 05:54:49.43 +46:08:44.5
165.98712 10.25551 galactic Aur Second-epoch detections are separated by 0.7" and 6.4 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 J088.6959+46.1467 | 05:54:49.43 +46:08:44.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.564+/-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 J088.6959+46.1467,2461129.6506,12.73,0.05,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 J088.6959+46.1467 20260330.1506 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:49.43 +46:08:44.5 ;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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1506 2461129.6506 12.85 06:01:16.71 +47:35:43.9
165.21221 11.91094 galactic Aur Second-epoch detections are separated by 1.6" and 5.9 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 | 06:01:16.71 +47:35:43.9 (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+47.5982,2461129.6506,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.3023+47.5982 20260330.1506 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:16.71 +47:35:43.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png resample_wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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_2026-03-29_22-37-09_20_00sec_-10_00C_LIGHT_0115_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_2026-03-29_22-36-09_20_00sec_-10_00C_LIGHT_0114_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: 2461129.65092111 30.03.2026 03:37:09.584 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
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: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 18251
Objects passed selection criteria: 18156
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 12957.2
Average stars matched: 12625.5 (97.4397 %)
Memory usage VmPeak: 124492 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 Sun Mar 29 22:41:18 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: 2461129.65092111 30.03.2026 03:37:09.584 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 147
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: 31 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): 132325
Objects passed selection criteria: 132017
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 102655
Average stars matched: 99206.8 (96.6412 %)
Memory usage VmPeak: 1902724 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 Sun Mar 29 22:43:39 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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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: 2461129.65023063
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
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_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits'
wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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 06:00:01.072 +46:00:27.20
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 06:00:04.553 +46:00:19.33
Angular distance between the image centers 0.05 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 06:00:01.072 +46:00:27.20
Second-epoch second image center 06:00:04.553 +46:00:19.33
Angular distance between the image centers 0.01031 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.AlByNXjbcu
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.Nsej7xInyh
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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits &> /tmp/tmp.ECpd9fpOXr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits &> /tmp/tmp.gZ8QT8Enuc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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 1 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
2.4 pix fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
2.4 pix fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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
14.1 mag. fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
14.1 mag. fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.AlByNXjbcu (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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/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.Nsej7xInyh (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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/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.ECpd9fpOXr (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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.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_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=617, passed=8303
Got 8303 stars (including 7677 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat
util/solve_plate_with_UCAC5 got 8303 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits -region wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.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.gZ8QT8Enuc (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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=615, passed=8186
Got 8186 stars (including 7563 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat
util/solve_plate_with_UCAC5 got 8186 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 933 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits -region wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/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_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits'
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31224.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31224_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 31224_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:34:27.50 +44:52:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.50, MAG_FAINT_SEARCH_LIMIT=11.48)GAIADR2_OUTPUT=# 0.772 207908784002418688 083.61485843374 +44.87196594922 10.2491 9.4244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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 06:00:01.072 +46:00:27.20
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 06:00:04.553 +46:00:19.33
Angular distance between the image centers 0.05 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 06:00:01.072 +46:00:27.20
Second-epoch second image center 06:00:04.553 +46:00:19.33
Angular distance between the image centers 0.01031 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.hexkCQU64H
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.lFSiIqqocb
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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits &> /tmp/tmp.PnXPLlQf80
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits &> /tmp/tmp.DJMAd9xnh5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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 123 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
2.0 pix fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
2.0 pix fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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
13.2 mag. fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
13.2 mag. fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hexkCQU64H (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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/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.lFSiIqqocb (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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/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.PnXPLlQf80 (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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.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_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=4210, passed=73507
Got 73507 stars (including 69199 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat
util/solve_plate_with_UCAC5 got 73507 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 938 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits -region wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.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.DJMAd9xnh5 (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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=4212, passed=73162
Got 73162 stars (including 68861 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat
util/solve_plate_with_UCAC5 got 73162 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.60"
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_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits -region wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/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_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-36-09_20.00sec_-10.00C_LIGHT_0114.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.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_2026-03-29_CI_Aur-02-Q2b1x1_223907_TTUQ2b1x1_15770_HHdzCkXv/wcs_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115.fits
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out193155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193185.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out193151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194274.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 49s
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: 20s
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Considering the candidate 193139_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193139_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:36:54.21 +45:40:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193148_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193148_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:40:46.51 +47:09:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193150_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193150_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:32:47.61 +44:25:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193151_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193151_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193155_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193155_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:57:24.99 +48:02:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.393 210174606884116224 089.35469408819 +48.04340148810 13.4268 12.4829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193160_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193160_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:34:24.10 +42:20:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193164_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193164_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193165_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193165_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:45:09.11 +48:42:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.358 211003569932468736 086.28895098594 +48.71376596592 13.5977 12.7663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193174_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193174_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193179_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193179_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:49:53.89 +47:59:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.278 210294969048402304 087.47548175815 +47.99534635235 13.7125 12.9240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193180_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193180_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193181_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193181_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:57:52.18 +48:46:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.453 210444502629100544 089.46842056173 +48.77710780595 13.7285 13.0185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193185_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193185_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:27:16.19 +45:33:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.486 208891717333926528 081.81826265908 +45.55967745585 13.5125 13.0409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193186_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193186_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:33:20.03 +43:46:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 1.510 195777464193169536 083.33398581104 +43.77914793737 13.4698 13.0100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193187_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193187_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193192_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193192_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:28:47.84 +44:55:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193198_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193198_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:28:35.73 +43:09:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193200_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193200_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:28:33.88 +44:21:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193206_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193206_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:31:57.78 +45:00:32.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)
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Considering the candidate 193208_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193208_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:31:33.12 +44:26:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.249 207873187313427200 082.88836538409 +44.43377129108 13.2904 12.7385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193211_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193211_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:42:01.63 +46:28:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.489 209646837008031616 085.50739242992 +46.47416496998 13.1824 12.4695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193220_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193220_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:11:13.00 +47:02:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.649 969416385483084800 092.80474694837 +47.04423121691 13.2454 12.7727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193221_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193221_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193222_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193222_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:34:42.36 +41:41:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193224_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193224_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:44:58.16 +47:20:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193226_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193226_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:37:02.78 +42:12:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193233_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193233_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193234_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193234_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 193235_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193235_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193238_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193238_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:35:48.01 +41:58:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193242_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193242_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:32:41.19 +42:27:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.744 194714545686194816 083.17152262380 +42.46547416906 12.8832 12.0416 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 193247_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193247_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193249_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193249_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193251_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193251_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193252_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193252_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:51:38.13 +48:20:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.470 210370418736729472 087.90946632657 +48.33580450234 12.7164 12.1774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193254_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193254_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:50:24.73 +41:49:10.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)
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Considering the candidate 193256_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193256_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:57:46.21 +43:34:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193259_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193259_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193261_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193261_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:26:48.06 +43:44:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193265_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193265_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:28:11.13 +45:21:58.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.48, MAG_FAINT_SEARCH_LIMIT=11.46)
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Considering the candidate 193348_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193348_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:59:43.39 +44:59:09.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 193351_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193351_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:38:28.47 +43:00:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193358_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193358_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:43:27.52 +42:19:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.10, MAG_FAINT_SEARCH_LIMIT=11.08)GAIADR2_OUTPUT=# 0.434 193022397288096512 085.86480449930 +42.32350876868 10.9773 10.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193362_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193362_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193485_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193485_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193508_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193508_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:11:34.49 +48:44:36.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193511_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193511_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193533_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193533_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193536_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193536_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193597_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193597_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:33:38.37 +45:26:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193598_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193598_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:46:26.46 +47:55:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 1.823 209974903788049920 086.61100294443 +47.91704234689 12.4908 11.9745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193675_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193675_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:06:21.21 +48:46:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.829 969866223177226368 091.58945434374 +48.77666602788 12.4108 11.4977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193693_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193693_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:32:51.78 +42:57:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193714_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193714_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193718_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193718_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:19:04.22 +47:21:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 0.587 968930641861363072 094.76769800520 +47.36474567364 12.5150 12.0779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193735_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193735_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:40:02.68 +50:02:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193745_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193745_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:37:17.65 +45:03:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193754_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193754_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:59:17.87 +44:58:17.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 193755_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193755_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:39:07.53 +44:53:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 1.382 197368109622667392 084.78191388712 +44.88670652218 12.6990 11.8738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193756_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193756_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:45:42.87 +43:37:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193761_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193761_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:34:37.50 +45:55:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193764_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193764_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:29:02.49 +42:56:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.591 195467848590572544 082.26096030690 +42.94394665295 12.8401 11.8496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193768_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193768_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:42:07.47 +50:04:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.699 214356977317827200 085.53219554945 +50.07566096651 13.0436 12.3953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193774_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193774_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:40:51.18 +48:19:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.295 210971134339379200 085.21413495392 +48.32280102290 12.9608 12.3722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193810_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193810_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193814_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193814_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:05:50.17 +44:39:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193828_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193828_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:49:02.48 +49:49:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.100 211485533981987968 087.26034393516 +49.83283336790 13.1234 12.2992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193842_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193842_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193853_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193853_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193879_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193879_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193884_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193884_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193885_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193885_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:57:46.07 +45:53:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.946 196952562947733504 089.44232599490 +45.88785721699 13.0324 12.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193889_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193889_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:57:08.46 +49:03:09.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193894_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193894_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:13:46.62 +44:43:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.616 962063465895464192 093.44440342022 +44.72742362945 12.6467 11.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193910_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193910_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:48:45.84 +46:35:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193917_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193917_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:47:16.23 +46:04:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.047 197524141490742528 086.81759006937 +46.07959594163 13.1672 12.3251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193946_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193946_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:59:52.53 +44:00:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.956 193367472142815360 089.96999756978 +44.00566216941 13.1290 12.3826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193963_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193963_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:40:25.82 +48:47:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.829 211054624206428800 085.10792870304 +48.79313041519 13.3541 12.6586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193972_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193972_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:38:38.22 +41:51:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193974_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 193974_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 193991_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193991_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:43:17.29 +42:28:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.714 193039675942126848 085.82223770632 +42.48052447032 12.9295 12.1211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193994_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193994_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:30:09.22 +46:12:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.772 209019462542689408 082.53951456145 +46.21579217952 13.5370 12.9587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193998_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 193998_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:40:42.92 +48:20:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.523 210971336200363648 085.17944784055 +48.33622155749 13.2097 12.6468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194011_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194011_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:49:32.53 +43:42:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.112 196476989808724224 087.38596124422 +43.70900222684 13.0460 12.1905 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 194034_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194034_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:11:00.96 +47:29:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194035_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194035_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:47:45.33 +50:03:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194043_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194043_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:30:56.99 +43:05:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194044_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194044_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:53:11.97 +45:24:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 2.211 196872028016249856 088.30074499759 +45.40620224136 13.2360 12.5061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194051_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194051_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:33:23.69 +43:46:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194052_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 194052_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 194056_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 194056_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 194059_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 194059_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 194060_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 194060_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 194062_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194062_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:32:58.08 +44:19:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194064_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194064_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:40:14.17 +50:00:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194081_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194081_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:33:56.38 +46:11:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194084_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194084_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:26:46.70 +44:21:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194088_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 194088_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 194092_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194092_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:31:00.40 +42:54:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194094_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 194094_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 194105_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194105_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:43:06.48 +44:51:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.904 197250427518440192 085.77769553460 +44.85885826898 13.2594 12.2721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194137_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 194137_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 194144_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194144_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:27:25.90 +44:48:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194171_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194171_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:52:03.60 +49:32:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.191 211244191180148352 088.01550768143 +49.54892102579 13.3825 12.6034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194190_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194190_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:44:48.17 +48:58:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194192_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194192_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:01:04.62 +50:00:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194195_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 194195_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 194196_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194196_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:00:13.90 +47:43:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.103 963734830944569856 090.05878481423 +47.72069134482 13.5637 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194216_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194216_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:34:02.85 +46:44:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194240_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 194240_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 194242_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194242_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:54:46.95 +46:08:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 0.819 197756344602976384 088.69592668878 +46.14675681897 13.1311 12.0714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194243_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194243_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:28:50.44 +44:16:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194245_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194245_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:38:46.38 +46:04:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.051 209541769223400064 084.69366740623 +46.06689801652 13.5146 12.8649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194253_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194253_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:24:59.28 +46:40:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194274_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
Preparing report for the candidate 194274_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
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Considering the candidate 194326_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194326_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:40:59.40 +46:21:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.866 209552042785104768 085.24823356916 +46.36291720392 13.8385 13.1940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194343_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194343_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:31:17.51 +46:25:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 0.118 209027850616719488 082.82299847399 +46.42981585602 13.7731 12.9103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194346_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194346_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:57:53.37 +46:05:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.445 197005378160950784 089.47179707530 +46.09439219961 14.0011 13.1854 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194357_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194357_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:38:50.29 +49:49:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194376_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 194376_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:39:18.36 +44:01:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.649 197062106090089600 084.82750509630 +44.02700003359 13.7838 13.2144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52500_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 52500_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:59:44.01 +47:37:00.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41230_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 41230_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 05:57:23.96 +48:22:40.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115
The candidate 63136_fd_Aur-02-Q2b1x1_2026-03-29_22-37-09_20.00sec_-10.00C_LIGHT_0115 did not pass the final checks
**** FOUND 06:14:59.00 +46:47:46.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 75s
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 ####
05:38:47.21 +45:24:51.0
05:53:45.51 +44:06:45.2
05:35:47.07 +43:12:12.8
05:29:09.68 +43:57:13.0
06:14:09.07 +44:09:21.9
05:30:25.33 +43:26:20.8
06:31:06.84 +48:10:19.5
06:19:17.98 +48:31:23.4
05:38:22.31 +42:05:46.6
05:41:49.15 +41:45:07.3
05:30:06.84 +42:29:53.2
05:57:09.05 +46:13:43.3
05:37:22.95 +46:49:17.9
05:26:36.91 +44:48:50.3
05:25:37.67 +45:40:56.8
05:39:19.47 +42:40:25.4
05:51:47.60 +48:44:50.8
06:15:03.58 +48:49:21.6
05:51:18.31 +46:14:40.9
05:48:04.00 +43:19:51.0
05:43:52.93 +47:06:14.7
05:35:42.02 +42:29:11.9
05:37:23.76 +47:29:29.9
06:26:58.99 +47:46:34.8
05:35:17.67 +42:18:25.8
05:26:06.50 +46:10:28.8
05:37:40.49 +43:34:43.9
05:40:17.40 +46:01:07.2
05:31:40.31 +42:51:24.2
05:28:11.60 +43:27:55.4
05:49:05.93 +45:12:36.2
05:37:46.19 +43:03:13.0
05:54:49.43 +46:08:44.5
06:01:16.71 +47:35:43.9
########### 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 ####
05:38:47.21 +45:24:51.0
05:53:45.51 +44:06:45.2
05:35:47.07 +43:12:12.8
05:29:09.68 +43:57:13.0
06:14:09.07 +44:09:21.9
05:30:25.33 +43:26:20.8
06:31:06.84 +48:10:19.5
06:19:17.98 +48:31:23.4
05:38:22.31 +42:05:46.6
05:41:49.15 +41:45:07.3
05:30:06.84 +42:29:53.2
05:57:09.05 +46:13:43.3
05:37:22.95 +46:49:17.9
05:26:36.91 +44:48:50.3
05:25:37.67 +45:40:56.8
05:39:19.47 +42:40:25.4
05:51:47.60 +48:44:50.8
06:15:03.58 +48:49:21.6
05:51:18.31 +46:14:40.9
05:48:04.00 +43:19:51.0
05:43:52.93 +47:06:14.7
05:35:42.02 +42:29:11.9
05:37:23.76 +47:29:29.9
06:26:58.99 +47:46:34.8
05:35:17.67 +42:18:25.8
05:26:06.50 +46:10:28.8
05:37:40.49 +43:34:43.9
05:40:17.40 +46:01:07.2
05:31:40.31 +42:51:24.2
05:28:11.60 +43:27:55.4
05:49:05.93 +45:12:36.2
05:37:46.19 +43:03:13.0
05:54:49.43 +46:08:44.5
06:01:16.71 +47:35:43.9
###################################################################################
05:38:47.21 +45:24:51.0 -- not an asteroid (will add it to exclusion list)
05:53:45.51 +44:06:45.2 -- not an asteroid (will add it to exclusion list)
05:35:47.07 +43:12:12.8 -- not an asteroid (will add it to exclusion list)
05:29:09.68 +43:57:13.0 -- not an asteroid (will add it to exclusion list)
06:14:09.07 +44:09:21.9 -- not an asteroid (will add it to exclusion list)
05:30:25.33 +43:26:20.8 -- not an asteroid (will add it to exclusion list)
06:31:06.84 +48:10:19.5 -- not an asteroid (will add it to exclusion list)
06:19:17.98 +48:31:23.4 -- not an asteroid (will add it to exclusion list)
05:38:22.31 +42:05:46.6 -- not an asteroid (will add it to exclusion list)
05:41:49.15 +41:45:07.3 -- not an asteroid (will add it to exclusion list)
05:30:06.84 +42:29:53.2 -- not an asteroid (will add it to exclusion list)
05:57:09.05 +46:13:43.3 -- not an asteroid (will add it to exclusion list)
05:37:22.95 +46:49:17.9 -- not an asteroid (will add it to exclusion list)
05:26:36.91 +44:48:50.3 -- not an asteroid (will add it to exclusion list)
05:25:37.67 +45:40:56.8 -- not an asteroid (will add it to exclusion list)
05:39:19.47 +42:40:25.4 -- not an asteroid (will add it to exclusion list)
05:51:47.60 +48:44:50.8 -- not an asteroid (will add it to exclusion list)
06:15:03.58 +48:49:21.6 -- not an asteroid (will add it to exclusion list)
05:51:18.31 +46:14:40.9 -- not an asteroid (will add it to exclusion list)
05:48:04.00 +43:19:51.0 -- not an asteroid (will add it to exclusion list)
05:43:52.93 +47:06:14.7 -- not an asteroid (will add it to exclusion list)
05:35:42.02 +42:29:11.9 -- not an asteroid (will add it to exclusion list)
05:37:23.76 +47:29:29.9 -- not an asteroid (will add it to exclusion list)
06:26:58.99 +47:46:34.8 -- not an asteroid (will add it to exclusion list)
05:35:17.67 +42:18:25.8 -- not an asteroid (will add it to exclusion list)
05:26:06.50 +46:10:28.8 -- not an asteroid (will add it to exclusion list)
05:37:40.49 +43:34:43.9 -- not an asteroid (will add it to exclusion list)
05:40:17.40 +46:01:07.2 -- not an asteroid (will add it to exclusion list)
05:31:40.31 +42:51:24.2 -- not an asteroid (will add it to exclusion list)
05:28:11.60 +43:27:55.4 -- not an asteroid (will add it to exclusion list)
05:49:05.93 +45:12:36.2 -- not an asteroid (will add it to exclusion list)
05:37:46.19 +43:03:13.0 -- not an asteroid (will add it to exclusion list)
05:54:49.43 +46:08:44.5 -- not an asteroid (will add it to exclusion list)
06:01:16.71 +47:35:43.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:25:37.67 +45:40:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:06.50 +46:10:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:36.91 +44:48:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:11.60 +43:27:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:09.68 +43:57:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:06.84 +42:29:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:25.33 +43:26:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:40.31 +42:51:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:17.67 +42:18:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:42.02 +42:29:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:47.07 +43:12:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:22.95 +46:49:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:23.76 +47:29:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:40.49 +43:34:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:46.19 +43:03:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:22.31 +42:05:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:47.21 +45:24:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:19.47 +42:40:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:17.40 +46:01:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:49.15 +41:45:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:52.93 +47:06:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:04.00 +43:19:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:05.93 +45:12:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.31 +46:14:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:47.60 +48:44:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:45.51 +44:06:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:49.43 +46:08:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:09.05 +46:13:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:16.71 +47:35:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:09.07 +44:09:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:03.58 +48:49:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:17.98 +48:31:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:58.99 +47:46:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:06.84 +48:10:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
05:25:37.67 +45:40:56.8 -- not a known variable star
05:26:06.50 +46:10:28.8 -- not a known variable star
05:26:36.91 +44:48:50.3 -- a known variable star
05:28:11.60 +43:27:55.4 -- not a known variable star
05:29:09.68 +43:57:13.0 -- not a known variable star
05:30:06.84 +42:29:53.2 -- a known variable star
05:30:25.33 +43:26:20.8 -- not a known variable star
05:31:40.31 +42:51:24.2 -- not a known variable star
05:35:17.67 +42:18:25.8 -- a known variable star
05:35:42.02 +42:29:11.9 -- not a known variable star
05:35:47.07 +43:12:12.8 -- not a known variable star
05:37:22.95 +46:49:17.9 -- not a known variable star
05:37:23.76 +47:29:29.9 -- not a known variable star
05:37:40.49 +43:34:43.9 -- not a known variable star
05:37:46.19 +43:03:13.0 -- not a known variable star
05:38:22.31 +42:05:46.6 -- not a known variable star
05:38:47.21 +45:24:51.0 -- not a known variable star
05:39:19.47 +42:40:25.4 -- not a known variable star
05:40:17.40 +46:01:07.2 -- not a known variable star
05:41:49.15 +41:45:07.3 -- not a known variable star
05:43:52.93 +47:06:14.7 -- not a known variable star
05:48:04.00 +43:19:51.0 -- not a known variable star
05:49:05.93 +45:12:36.2 -- not a known variable star
05:51:18.31 +46:14:40.9 -- not a known variable star
05:51:47.60 +48:44:50.8 -- not a known variable star
05:53:45.51 +44:06:45.2 -- not a known variable star
05:54:49.43 +46:08:44.5 -- not a known variable star
05:57:09.05 +46:13:43.3 -- not a known variable star
06:01:16.71 +47:35:43.9 -- not a known variable star
06:14:09.07 +44:09:21.9 -- not a known variable star
06:15:03.58 +48:49:21.6 -- not a known variable star
06:19:17.98 +48:31:23.4 -- not a known variable star
06:26:58.99 +47:46:34.8 -- not a known variable star
06:31:06.84 +48:10:19.5 -- not a known variable star
Found 31 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
34 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
05:25:37.67 +45:40:56.8
05:26:06.50 +46:10:28.8
05:26:36.91 +44:48:50.3
05:28:11.60 +43:27:55.4
05:29:09.68 +43:57:13.0
05:30:06.84 +42:29:53.2
05:30:25.33 +43:26:20.8
05:31:40.31 +42:51:24.2
05:35:17.67 +42:18:25.8
05:35:42.02 +42:29:11.9
05:35:47.07 +43:12:12.8
05:37:22.95 +46:49:17.9
05:37:23.76 +47:29:29.9
05:37:40.49 +43:34:43.9
05:37:46.19 +43:03:13.0
05:38:22.31 +42:05:46.6
05:38:47.21 +45:24:51.0
05:39:19.47 +42:40:25.4
05:40:17.40 +46:01:07.2
05:41:49.15 +41:45:07.3
05:43:52.93 +47:06:14.7
05:48:04.00 +43:19:51.0
05:49:05.93 +45:12:36.2
05:51:18.31 +46:14:40.9
05:51:47.60 +48:44:50.8
05:53:45.51 +44:06:45.2
05:54:49.43 +46:08:44.5
05:57:09.05 +46:13:43.3
06:01:16.71 +47:35:43.9
06:14:09.07 +44:09:21.9
06:15:03.58 +48:49:21.6
06:19:17.98 +48:31:23.4
06:26:58.99 +47:46:34.8
06:31:06.84 +48:10:19.5
05:34:27.50 +44:52:19.4
05:57:24.99 +48:02:36.5
05:45:09.11 +48:42:49.6
05:49:53.89 +47:59:43.0
05:57:52.18 +48:46:37.0
05:27:16.19 +45:33:33.4
05:33:20.03 +43:46:44.3
06:31:57.78 +45:00:32.1
05:31:33.12 +44:26:02.4
05:42:01.63 +46:28:27.0
06:11:13.00 +47:02:38.4
05:32:41.19 +42:27:56.4
05:51:38.13 +48:20:08.5
05:50:24.73 +41:49:10.6
05:28:11.13 +45:21:58.8
05:43:27.52 +42:19:24.4
05:46:26.46 +47:55:01.2
06:06:21.21 +48:46:37.2
06:19:04.22 +47:21:53.6
05:39:07.53 +44:53:12.0
05:29:02.49 +42:56:38.6
05:42:07.47 +50:04:31.3
05:40:51.18 +48:19:21.2
05:49:02.48 +49:49:57.1
05:57:46.07 +45:53:16.5
06:13:46.62 +44:43:39.2
05:47:16.23 +46:04:44.5
05:59:52.53 +44:00:17.7
05:40:25.82 +48:47:35.4
05:43:17.29 +42:28:49.4
05:30:09.22 +46:12:56.4
05:40:42.92 +48:20:10.0
05:49:32.53 +43:42:32.2
05:53:11.97 +45:24:22.1
05:43:06.48 +44:51:31.2
05:52:03.60 +49:32:56.0
06:00:13.90 +47:43:14.5
05:54:46.95 +46:08:48.0
05:38:46.38 +46:04:00.7
05:40:59.40 +46:21:46.1
05:31:17.51 +46:25:47.4
05:57:53.37 +46:05:39.9
05:39:18.36 +44:01:36.7
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461129.65023063 -observatory 500
22:54:37.34 -08:02:10.8 Mercury (0.5mag)
01:48:33.34 +10:37:49.9 Venus (-3.9mag)
23:29:41.92 -04:24:49.3 Mars (1.2mag)
07:06:34.81 +22:55:35.0 Jupiter (-2.2mag)
00:21:32.61 +00:00:46.6 Saturn (0.9mag)
03:44:25.87 +19:36:51.4 Uranus (5.8mag)
00:08:33.71 -00:29:51.0 Neptune (7.8mag)
20:32:45.35 -22:52:50.1 Pluto (14.5mag)
10:24:24.25 +10:23:14.5 Moon (-11.8mag)
-rw-r--r-- 1 apache apache 362 Mar 29 22:41 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461129.65023063:
07:06:37.70 +22:55:26.7 Io (5.7mag)
07:06:47.40 +22:55:09.0 Europa (5.8mag)
07:06:31.09 +22:55:49.7 Ganymede (5.2mag)
07:07:11.65 +22:54:26.2 Callisto (6.5mag)
07:10:29.21 +22:51:56.0 Himalia (15.2mag)
07:06:36.42 +22:55:29.3 Thebe (16.1mag)
07:10:16.49 +23:18:45.7 Elara (17.2mag)
07:04:19.11 +23:44:25.6 Pasiphae (17.3mag)
07:15:14.09 +22:51:33.5 Carme (18.4mag)
00:21:36.98 +00:01:07.0 Titan (8.8mag)
00:21:37.59 +00:00:47.2 Rhea (10.1mag)
00:21:48.74 +00:02:53.8 Iapetus (11.5mag)
00:21:24.58 +00:01:10.9 Hyperion (14.8mag)
00:23:21.49 +00:11:15.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 29 22:41 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461129.65023063:
14:00:23.64 -01:05:37.3 JWST
18:19:01.22 +30:06:37.1 Chandra
16:22:19.74 -52:30:48.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 29 22:41 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461129.65023063 -observatory 500
18:42:33.33 -27:52:58.4 14.0mag P/2010 H2 (Vales)
04:55:52.03 -70:31:19.4 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:33.90 +31:20:19.8 17.1mag C/2017 K2 (PANSTARRS)
17:30:42.41 +08:30:49.3 17.6mag C/2021 G2 (ATLAS)
23:04:58.57 +28:39:07.4 17.0mag C/2022 E2 (ATLAS)
04:10:12.08 +25:33:37.3 15.8mag C/2022 N2 (PANSTARRS)
09:01:28.79 +31:45:07.7 16.1mag C/2022 QE78 (ATLAS)
08:29:46.08 -02:03:25.3 17.2mag C/2022 R6 (PANSTARRS)
18:56:18.50 +17:04:59.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:02.95 -11:44:58.8 17.6mag P/2023 B1 (PANSTARRS)
09:17:26.99 -14:43:04.4 17.5mag C/2023 F3 (ATLAS)
21:34:37.07 +62:02:39.6 17.4mag C/2023 H5 (Lemmon)
19:30:04.08 -03:33:28.0 14.4mag C/2023 R1 (PANSTARRS)
21:42:08.18 +83:46:47.5 17.8mag C/2023 X2 (Lemmon)
06:13:50.13 +63:39:49.1 16.9mag C/2024 A1 (ATLAS)
04:33:11.70 +11:04:41.7 9.9mag C/2024 E1 (Wierzchos)
16:28:36.59 +03:37:37.3 17.4mag C/2024 G6 (ATLAS)
20:14:34.97 +10:55:26.7 14.8mag C/2024 J3 (ATLAS)
03:11:53.76 -25:04:57.3 16.4mag C/2024 T5 (ATLAS)
05:03:28.12 +49:48:58.4 17.6mag C/2025 J1 (Borisov)
14:45:25.76 +29:27:33.0 14.6mag C/2025 L1 (ATLAS)
03:00:27.12 -23:46:31.2 17.7mag C/2025 Q3 (ATLAS)
22:40:58.93 +19:36:15.0 11.2mag C/2025 R3 (PANSTARRS)
13:01:24.02 +01:55:29.9 17.6mag C/2025 Y1 (ATLAS)
01:39:48.38 -00:10:28.2 11.1mag C/2026 A1 (MAPS)
23:08:54.05 +33:34:32.9 14.0mag C/2026 B2 (Sun-Gao)
18:10:00.19 -10:31:33.1 12.8mag 10P/Tempel
15:20:19.61 +04:37:03.9 12.5mag 24P/Schaumasse
11:08:18.64 -02:07:39.2 15.7mag 29P/Schwassmann-Wachmann
17:51:58.54 -10:16:54.4 17.5mag 40P/Vaisala
10:41:01.10 -05:37:55.7 16.6mag 43P/Wolf-Harrington
01:22:47.90 +14:33:27.4 17.1mag 47P/Ashbrook-Jackson
06:41:51.68 +40:31:09.8 17.1mag 63P/Wild
23:06:51.12 -13:32:59.4 15.7mag 65P/Gunn
03:20:10.60 +15:01:55.8 15.9mag 76P/West-Kohoutek-Ikemura
00:28:54.86 +04:52:38.8 14.5mag 78P/Gehrels
22:09:41.09 -14:16:41.5 14.5mag 88P/Howell
01:24:21.03 +15:55:30.3 15.2mag 93P/Lovas
04:24:58.04 +31:17:13.1 16.4mag 123P/West-Hartley
08:12:13.67 +46:07:45.6 16.2mag 124P/Mrkos
02:07:41.52 +12:26:13.0 16.4mag 128P/Shoemaker-Holt
02:14:49.37 +12:18:41.1 17.4mag 131P/Mueller
00:01:45.13 +06:47:51.0 11.9mag 141P/Machholz
00:12:00.61 -01:21:00.1 12.0mag 141P-A/Machholz
23:06:53.80 -04:31:41.4 14.9mag 141P-D/Machholz
00:15:41.34 -09:50:41.4 15.3mag 162P/SidingSpring
10:33:52.54 +31:50:42.1 17.7mag 164P/Christensen
06:05:43.09 +24:39:13.5 17.7mag 198P/ODAS
15:20:17.82 -02:07:07.6 17.2mag 210P/Christensen
20:45:17.43 -15:29:47.3 17.3mag 218P/LINEAR
17:07:47.91 -15:49:14.7 16.2mag 235P/LINEAR
04:59:16.77 +33:07:05.2 16.5mag 240P/NEAT
07:31:52.49 -07:09:44.3 17.6mag 242P/Spahr
15:47:32.08 +05:47:21.1 17.6mag 391P/Kowalski
07:29:15.06 +21:14:25.1 17.6mag 450P/LONEOS
05:12:26.84 +46:02:16.0 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Mar 29 22:41 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 29 22:41 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 29 22:41 tocp_transients_list.txt