This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ
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 02 27.3476 2461098.8476 11.71 16:33:27.28 +25:55:17.5
44.87480 40.74246 galactic Her Second-epoch detections are separated by 1.4" and 5.2 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 J248.3578+25.9292 | 16:33:26.58 +25:55:17.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 33 27.28 +25 55 17.5 11.7 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J248.3578+25.9292,2461098.8476,11.71,0.05,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 J248.3578+25.9292 20260227.3476 11.71CV 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/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:33:27.28 +25:55:17.5 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 14.06 16:29:06.17 +24:57:34.6
43.30799 41.44695 galactic Her Second-epoch detections are separated by 6.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:29:06.17 +24:57:34.6 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 29 06.17 +24 57 34.6 14.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.8476,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.3476 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:29:06.17 +24:57:34.6 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 32 11.28 +25 59 50.5 14.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.8476,14.04,0.05,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
target 20260227.3476 14.04CV 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/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:32:11.28 +25:59:50.5 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.93 16:30:39.09 +25:34:21.1
44.21682 41.26560 galactic Her Second-epoch detections are separated by 2.5" and 4.9 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 | 16:30:39.09 +25:34:21.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 30 39.09 +25 34 21.1 13.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.8476,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.3476 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:30:39.09 +25:34:21.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.74 16:34:24.09 +28:25:24.4
48.16035 41.12114 galactic Her Second-epoch detections are separated by 0.9" and 5.0 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 1305660162379380096 | 16:34:24.69 +28:25:24.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 34 24.09 +28 25 24.4 13.7 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1305660162379380096,2461098.8476,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1305660162379380096 20260227.3476 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:34:24.09 +28:25:24.4 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.63 16:31:06.50 +25:53:13.5
44.65618 41.24482 galactic Her Second-epoch detections are separated by 2.5" and 5.0 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 | Large-amplitude variable Gaia DR2 1304023028220536064 | 16:31:06.02 +25:53:13.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 31 06.50 +25 53 13.5 13.6 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1304023028220536064,2461098.8476,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1304023028220536064 20260227.3476 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:31:06.50 +25:53:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.46 16:31:55.63 +25:22:06.1
44.05213 40.93517 galactic Her Second-epoch detections are separated by 5.5" 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 1303844078407910016 | 16:31:55.07 +25:22:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 31 55.63 +25 22 06.1 13.5 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1303844078407910016,2461098.8476,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1303844078407910016 20260227.3476 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:31:55.63 +25:22:06.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.24 16:33:39.91 +26:35:59.4
45.75873 40.86344 galactic Her Second-epoch detections are separated by 1.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1304446408918692864 | 16:33:39.12 +26:35:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 33 39.91 +26 35 59.4 13.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1304446408918692864,2461098.8476,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1304446408918692864 20260227.3476 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:33:39.91 +26:35:59.4 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.17 16:29:59.46 +25:30:05.5
44.07518 41.39180 galactic Her Second-epoch detections are separated by 3.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1303904658923521664 | 16:29:59.99 +25:30:02.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 29 59.46 +25 30 05.5 13.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1303904658923521664,2461098.8476,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1303904658923521664 20260227.3476 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:29:59.46 +25:30:05.5 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.24 16:31:51.09 +25:24:18.8
44.09350 40.96115 galactic Her Second-epoch detections are separated by 1.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1303856005533948160 | 16:31:50.48 +25:24:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 31 51.09 +25 24 18.8 13.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1303856005533948160,2461098.8476,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1303856005533948160 20260227.3476 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:31:51.09 +25:24:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.19 16:33:39.54 +26:50:26.0
46.06748 40.92240 galactic Her Second-epoch detections are separated by 0.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J248.4099+26.8370 | 16:33:38.70 +26:50:26.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 33 39.54 +26 50 26.0 13.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J248.4099+26.8370,2461098.8476,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J248.4099+26.8370 20260227.3476 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:33:39.54 +26:50:26.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.10 16:31:20.32 +25:19:21.3
43.94828 41.05192 galactic Her Second-epoch detections are separated by 2.4" and 5.3 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 1303853978309387904 | 16:31:19.79 +25:19:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 31 20.32 +25 19 21.3 13.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1303853978309387904,2461098.8476,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1303853978309387904 20260227.3476 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:31:20.32 +25:19:21.3 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.10 16:33:48.80 +25:40:17.5
44.58272 40.60124 galactic Her Second-epoch detections are separated by 2.3" and 4.6 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 1303945959329454464 | 16:33:49.28 +25:40:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 33 48.80 +25 40 17.5 13.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1303945959329454464,2461098.8476,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1303945959329454464 20260227.3476 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:33:48.80 +25:40:17.5 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 12.82 16:31:02.51 +25:06:04.4
43.64169 41.05961 galactic Her Second-epoch detections are separated by 1.9" and 5.0 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 1303832159876115456 | 16:31:01.93 +25:06:05.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 31 02.51 +25 06 04.4 12.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1303832159876115456,2461098.8476,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1303832159876115456 20260227.3476 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:31:02.51 +25:06:04.4 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 12.39 16:30:26.73 +25:10:24.6
43.68798 41.20868 galactic Her Second-epoch detections are separated by 1.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1303822573508452096 | 16:30:26.18 +25:10:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 30 26.73 +25 10 24.6 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1303822573508452096,2461098.8476,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1303822573508452096 20260227.3476 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:30:26.73 +25:10:24.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 12.33 16:34:08.07 +26:35:07.2
45.77361 40.75812 galactic Her Second-epoch detections are separated by 2.5" and 5.3 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 1304434039412872960 | 16:34:07.31 +26:35:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3476* 16 34 08.07 +26 35 07.2 12.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1304434039412872960,2461098.8476,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1304434039412872960 20260227.3476 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:34:08.07 +26:35:07.2 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3476 2461098.8476 13.85 16:05:46.58 +33:11:02.1
53.43240 47.92764 galactic CrB Second-epoch detections are separated by 3.1" and 4.3 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 1323191432904175360 | 16:05:44.34 +33:11:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.599+/-0.036 (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 1323191432904175360,2461098.8476,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1323191432904175360 20260227.3476 13.85CV 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/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:05:46.58 +33:11:02.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_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
Z CrB,2461098.8476,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Z CrB 20260227.3476 9.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:56:08.46 +29:14:17.7 ;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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20_00sec_-14_90C_LIGHT_0104_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: 2461033.02132514 23.12.2025 12:30:32.492 /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
First image: 2461033.02132514 23.12.2025 12:30:32.492 /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
Last image: 2461098.84791433 27.02.2026 08:20:49.798 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 28
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
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: 2 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): 7137
Objects passed selection criteria: 7125
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 6431.25
Average stars matched: 6289.5 (97.7959 %)
Memory usage VmPeak: 113136 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Feb 27 04:37:45 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461033.02132514 23.12.2025 12:30:32.492 /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
First image: 2461033.02132514 23.12.2025 12:30:32.492 /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
Last image: 2461098.84791433 27.02.2026 08:20:49.798 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 112
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
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: 12 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): 40341
Objects passed selection criteria: 40271
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 37050
Average stars matched: 35465.2 (95.7227 %)
Memory usage VmPeak: 142352 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Feb 27 04:38:45 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE=
FRAME_EDGE_OFFSET_PIX= 100
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
CrB-02-Q2b1x1
#######################################
########### Starting CrB-02-Q2b1x1 ###########
Processing CrB-02-Q2b1x1
server tau has sufficient free disk space available: 688557 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 688557 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.png' -> 'transient_report/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits_preview.png'
CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
renamed 'CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.png' -> 'transient_report/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits_preview.png'
CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 776.1834
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 534.8627
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1939.8449
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 615.8832
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1932.9524
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 615.5316
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.49921
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
SExtractor catalog cache: saved CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat to cache
SExtractor catalog cache: saved CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.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/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461098.84735931
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits exists and is non-empty
Saving wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits to local_wcs_cache/
'wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits' -> 'local_wcs_cache/wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits'
wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits exists and is non-empty
Saving wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits to local_wcs_cache/
'wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits' -> 'local_wcs_cache/wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits'
wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits exists and is non-empty
Saving wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits to local_wcs_cache/
'wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits' -> 'local_wcs_cache/wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits'
wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits exists and is non-empty
Saving wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits to local_wcs_cache/
'wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits' -> 'local_wcs_cache/wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:00:00.621 +29:59:51.60
Second-epoch image center 16:00:05.349 +29:57:45.15
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 16:00:00.621 +29:59:51.60
Second-epoch image center 16:00:07.283 +29:57:57.36
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:00:05.349 +29:57:45.15
Second-epoch second image center 16:00:07.283 +29:57:57.36
Angular distance between the image centers 0.00776 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/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits &> /tmp/tmp.Bc9txqYHFI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits &> /tmp/tmp.gvJQ8OsCEM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits &> /tmp/tmp.eWwGQdSpDt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits &> /tmp/tmp.9go2qvaRNg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits and wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits and wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat
Found non-empty wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits and wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat
The reference image (wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits) and catalog (wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat) found
'wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.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 4987 out of 7301 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.909124
a=0.000000 b=1.000000 c=22.909124
From vast_summary.log: estimated ref. image limiting mag.: -7.72
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.19
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 28 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
2.1 pix CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
2.4 pix CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
2.4 pix CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
Limiting magnitude estimates:
15.2 mag. CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
15.2 mag. CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
14.8 mag. CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
14.7 mag. CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Bc9txqYHFI (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/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits' -> 'wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
WCS_IMAGE_NAME=wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
WCS-calibrated image found: wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
Checking if the catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits alredy exist and is non-empty...
Catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
WCS catalog name: wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=433, passed=7301
Got 7301 stars (including 6853 good ones) from the SExtractor catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat
util/solve_plate_with_UCAC5 got 7301 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits -region wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.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.gvJQ8OsCEM (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/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits' -> 'wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
WCS_IMAGE_NAME=wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
WCS-calibrated image found: wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
Checking if the catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits alredy exist and is non-empty...
Catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
WCS catalog name: wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=490, passed=7353
Got 7353 stars (including 6849 good ones) from the SExtractor catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat
util/solve_plate_with_UCAC5 got 7353 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits -region wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.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.eWwGQdSpDt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
WCS_IMAGE_NAME=wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
WCS-calibrated image found: wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
Checking if the catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits alredy exist and is non-empty...
Catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
WCS catalog name: wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=437, passed=5602
Got 5602 stars (including 5162 good ones) from the SExtractor catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat
util/solve_plate_with_UCAC5 got 5602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits -region wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.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.9go2qvaRNg (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
WCS_IMAGE_NAME=wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
WCS-calibrated image found: wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
Checking if the catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits alredy exist and is non-empty...
Catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
WCS catalog name: wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=435, passed=5646
Got 5646 stars (including 5210 good ones) from the SExtractor catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat
util/solve_plate_with_UCAC5 got 5646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits -region wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field CrB-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20373.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20372_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20372_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:11:39.50 +30:15:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.548 1318779672566752512 242.91383465426 +30.25148210542 12.3562 11.8759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20373_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 20373_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 20378_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20378_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:56:08.46 +29:14:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.72, MAG_FAINT_SEARCH_LIMIT=10.70)GAIADR2_OUTPUT=# 0.567 1320011232960243072 239.03507472366 +29.23828725736 10.4967 9.3689 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20412_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20412_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:29:07.79 +34:13:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20417_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20417_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:22:31.35 +33:43:47.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20442_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20442_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:01:24.15 +30:24:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.167 1320564630905689728 240.35059818106 +30.41265431219 12.2455 11.7180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20443_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20443_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:48:53.41 +29:43:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.206 1320975229779781376 237.22255997805 +29.73324929737 12.0818 11.5296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20445_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20445_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:02:27.73 +29:25:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.318 1320178564885591168 240.61552964013 +29.42394008723 12.2330 11.7306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20448_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20448_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:52:01.32 +28:51:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.154 1319939936503077632 238.00550896357 +28.86012551158 11.9839 11.1685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20450_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20450_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:51:34.47 +31:26:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.674 1321617207130840832 237.89383746598 +31.44317530065 12.0896 11.5113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20451_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20451_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:00:14.28 +28:48:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.280 1319762331015553536 240.05958369369 +28.81225151949 12.0855 11.4069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20452_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20452_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:56:19.92 +29:46:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.190 1320110635683520768 239.08305122711 +29.77569524400 12.1151 11.3560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20453_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20453_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:58:43.28 +29:20:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.199 1320024839416784256 239.68031248233 +29.34383656113 12.2226 11.6240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20454_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20454_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:55:20.41 +28:10:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.306 1319655472229362560 238.83513167783 +28.16869732039 12.1973 11.6629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20455_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20455_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:53:31.92 +27:44:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.058 1223564718671591040 238.38298754373 +27.73776180896 11.3526 10.1478 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20456_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20456_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:56:37.46 +28:07:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.169 1319664096523644416 239.15606586033 +28.12809469182 12.1649 11.5170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20457_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20457_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:53:14.54 +29:01:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.344 1319963335484888576 238.31066845576 +29.01803207311 12.1511 11.5720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20462_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20462_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:00:57.72 +31:00:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.704 1320668015062379392 240.24063839768 +31.01515021162 12.3274 11.8838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20463_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20463_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:59:44.80 +30:24:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.318 1320520547362159232 239.93676597302 +30.40810462292 12.3696 11.9771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20465_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20465_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:00:31.42 +27:46:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.224 1316673150017527936 240.13098166167 +27.77467044123 12.1111 11.3636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20470_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20470_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:59:17.02 +28:06:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.655 1319698937298104576 239.82080173022 +28.11417897259 12.2347 11.7204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20472_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20472_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:03:21.79 +28:04:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.930 1316662567218176512 240.84074855177 +28.07819987664 12.2936 11.8157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20477_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20477_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:54:59.09 +29:19:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.564 1320061874917609600 238.74602882996 +29.31919207824 12.3863 11.9077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20480_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20480_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:06:47.87 +29:09:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.201 1317241318354736000 241.69939443974 +29.16060807015 12.1919 11.4704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20482_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20482_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:01:35.32 +32:25:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.154 1323058563796346240 240.39717184887 +32.42717960963 12.3280 11.8492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20485_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20485_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:50:18.41 +30:00:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.617 1321009898755921408 237.57687210110 +30.00937406983 12.3819 11.9681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20486_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20486_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:25:52.92 +24:48:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.428 1302347475581024768 246.47056906755 +24.81628784504 11.5291 10.9742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20492_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 20492_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:58:01.56 +27:28:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.272 1316559178766423936 239.50651863758 +27.47815709303 12.1736 11.4876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 13s
Prepared the HTML report for the field CrB-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 ####
16:33:27.28 +25:55:17.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
SExtractor catalog cache: saved CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat to cache
SExtractor catalog cache: saved CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
Creating symlink local_wcs_cache/wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
Creating symlink local_wcs_cache/wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
Creating symlink local_wcs_cache/wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits exists and is non-empty
wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits exists and is non-empty
wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits exists and is non-empty
wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:00:00.621 +29:59:51.60
Second-epoch image center 16:00:05.349 +29:57:45.15
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 16:00:00.621 +29:59:51.60
Second-epoch image center 16:00:07.283 +29:57:57.36
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:00:05.349 +29:57:45.15
Second-epoch second image center 16:00:07.283 +29:57:57.36
Angular distance between the image centers 0.00776 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/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits &> /tmp/tmp.z6c4wG0yOz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits &> /tmp/tmp.v0hVFcnOho
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits &> /tmp/tmp.cJteKqVw15
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits &> /tmp/tmp.syT7Sx94rm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits and wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.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_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits and wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat
Found non-empty wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits and wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat
The reference image (wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits) and catalog (wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat) found
'wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.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 5100 out of 42971 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.787050
a=0.000000 b=1.000000 c=22.787050
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 72 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
2.0 pix CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
2.4 pix CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
2.4 pix CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
Limiting magnitude estimates:
15.3 mag. CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
15.3 mag. CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
14.9 mag. CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
14.9 mag. CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.z6c4wG0yOz (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/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits' -> 'wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
WCS_IMAGE_NAME=wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
WCS-calibrated image found: wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
Checking if the catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits alredy exist and is non-empty...
Catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits
WCS catalog name: wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1818, passed=42962
Got 42962 stars (including 41065 good ones) from the SExtractor catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat
util/solve_plate_with_UCAC5 got 42962 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits -region wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.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.v0hVFcnOho (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/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits' -> 'wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
WCS_IMAGE_NAME=wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
WCS-calibrated image found: wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
Checking if the catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits alredy exist and is non-empty...
Catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits
WCS catalog name: wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1779, passed=42643
Got 42643 stars (including 40796 good ones) from the SExtractor catalog wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat
util/solve_plate_with_UCAC5 got 42643 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits -region wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-02-Q2b1x1_2025-12-23_06-31-22_20.00sec_-15.00C_LIGHT_0695.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.cJteKqVw15 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
WCS_IMAGE_NAME=wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
WCS-calibrated image found: wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
Checking if the catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits alredy exist and is non-empty...
Catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits
WCS catalog name: wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1449, passed=31657
Got 31657 stars (including 30172 good ones) from the SExtractor catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat
util/solve_plate_with_UCAC5 got 31657 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits -region wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-01_20.00sec_-14.90C_LIGHT_0104.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.syT7Sx94rm (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
WCS_IMAGE_NAME=wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
WCS-calibrated image found: wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
Checking if the catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits alredy exist and is non-empty...
Catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat corresponding to the image wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits
WCS catalog name: wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1491, passed=32008
Got 32008 stars (including 30485 good ones) from the SExtractor catalog wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat
util/solve_plate_with_UCAC5 got 32008 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_CrB-02-Q2b1x1_043512_TTUQ2b1x1_669_MOUtUjnJ/CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits -region wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field CrB-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out18409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54053.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 34s
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: 12s
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Considering the candidate 53262_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53262_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:36:50.65 +32:50:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 3.140 1324853963204947072 249.21183997476 +32.84130768634 13.4552 13.0311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53269_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53269_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:33:34.26 +34:08:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 3.212 1325941586363377408 248.39380855548 +34.14830796283 13.3008 12.6896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53270_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53270_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:27:28.63 +34:05:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.799 1278644203908660992 231.86940659664 +34.08341052018 13.7518 13.2803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53271_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53271_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:34:29.94 +28:10:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.986 1304878242110213376 248.62505823417 +28.17388213274 13.3358 12.8977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53272_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53272_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:30:53.52 +26:06:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.874 1304035294649199232 247.72388179521 +26.10667579039 13.0197 12.3759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53274_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53274_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:28:39.53 +25:33:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 2.260 1303897232923499136 247.16403426543 +25.56031579891 12.7826 12.0416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53276_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53276_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:31:41.72 +28:36:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.788 1305705727689353472 247.92438813461 +28.61512418215 13.2234 12.6679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53282_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53282_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:36:20.56 +32:13:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 4.595 1324682370671994112 249.08541724934 +32.21624105196 13.1117 12.7004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53285_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53285_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:22:12.08 +25:12:25.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)
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Considering the candidate 53287_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53287_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53290_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53290_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:26:00.57 +25:07:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.126 1302564148091316352 246.50247686935 +25.12130568372 12.7237 11.9964 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53293_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53293_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:33:03.22 +24:52:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.834 1300808773480228224 248.26316243311 +24.86964565654 12.4830 11.9047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53296_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53296_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 53297_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53297_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:21:01.32 +24:54:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 3.923 1302508931992017408 245.25668942906 +24.90229176371 13.0552 12.5430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53298_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53298_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:30:18.51 +25:57:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 3.150 1304026910873037696 247.57808278716 +25.96559419674 12.9145 12.4044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53299_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53299_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:33:27.11 +26:50:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.665 1304645798479881728 248.36271394939 +26.83915777821 12.5950 11.9286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53301_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53301_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 53302_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53302_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53303_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53303_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:05:20.20 +33:16:56.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)
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Considering the candidate 53305_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53305_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:33:19.87 +26:41:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.249 1304451008826995584 248.33185412804 +26.69641927600 12.5392 11.8348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53309_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53309_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53313_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53313_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:32:47.26 +25:56:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.374 1304038387025859840 248.19754266684 +25.94976038656 12.4911 11.8398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53314_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53314_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53317_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53317_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 53320_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53320_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:03:51.36 +33:14:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.705 1323204180367088256 240.96412790786 +33.24189143088 13.6946 13.2418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53322_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53322_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:31:31.26 +27:13:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.013 1304715269574894848 247.88024267000 +27.22742022970 12.7150 12.2133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53328_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53328_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53329_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53329_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:33:47.71 +26:02:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.535 1303998873326633344 248.44887847870 +26.04550243881 12.2221 11.8072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53330_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53330_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:31:53.67 +25:54:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 4.328 1304016568591759488 247.97496155585 +25.90427689942 12.3256 11.9033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53332_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53332_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:11:04.15 +31:29:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.015 1322008289673546368 242.76762062419 +31.49200044523 13.5917 13.0513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53333_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53333_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:22:00.67 +24:51:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.328 1302500445136612608 245.50208140634 +24.85322542950 12.4789 12.0184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53334_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53334_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53335_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53335_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:33:54.63 +27:44:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 5.116 1304852231788078080 248.47894587885 +27.75069685098 12.3301 11.8213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53336_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53336_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 53337_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53337_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 53338_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53338_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 53339_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53339_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 53340_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53340_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53341_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53341_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53345_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53345_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:28:48.92 +26:05:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.896 1304138476943382784 247.20295030130 +26.09128219174 11.9130 11.2577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53346_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53346_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53347_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53347_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53348_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53348_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53351_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53351_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53352_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53352_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 53354_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53354_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:32:54.95 +26:33:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.511 1304073159081053696 248.22893079308 +26.56197303512 11.6188 11.0400 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53357_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53357_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53362_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53362_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:30:39.35 +26:03:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 3.435 1304029316054723968 247.66289938904 +26.05775819471 11.2371 10.5916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53363_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53363_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:34:07.06 +28:16:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 4.233 1305633263000912256 248.53072740900 +28.26905434220 11.2877 10.6498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53368_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53368_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53369_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 53369_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 53371_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53371_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:48:50.90 +30:36:43.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)
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Considering the candidate 53372_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53372_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:31:24.60 +25:50:29.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53439_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53439_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:22:31.36 +33:43:47.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53543_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53543_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:25:52.93 +24:48:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.279 1302347475581024768 246.47056906755 +24.81628784504 11.5291 10.9742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53584_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53584_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:11:43.90 +33:22:06.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53893_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53893_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:49:39.70 +28:13:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.868 1223837084020994944 237.41568728795 +28.22029846667 13.6622 12.5479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53973_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 53973_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:11:32.55 +33:06:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.389 1322720704488651776 242.88541691376 +33.10146124828 14.0426 13.3843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54038_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 54038_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:47:39.22 +28:27:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.762 1224588329637708032 236.91338597940 +28.45014976886 14.3436 13.8641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54048_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 54048_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:23:16.54 +32:49:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 3.465 1325515972284526336 245.81831128917 +32.83032183348 14.1659 13.7532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54053_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 54053_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 54065_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 54065_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:38:48.29 +28:10:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.645 1224398732600920192 234.70060993002 +28.16659976128 14.0309 13.3542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54073_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 54073_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:01:51.22 +31:53:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.291 1322960844700339072 240.46394933582 +31.88525342515 14.1330 13.6355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54126_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 54126_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:43:55.13 +29:11:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.302 1224912891725625984 235.98007225946 +29.18968803355 13.8998 13.4729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54195_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 54195_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:37:08.77 +34:07:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.735 1326669359981838848 249.28711349052 +34.12981243739 13.4207 12.8506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54353_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 54353_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:01:39.30 +30:38:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.682 1320574423431133568 240.41321082060 +30.63444393421 15.0851 14.4150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54360_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 54360_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 15:59:12.55 +33:16:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.939 1323346842001046784 239.80232897974 +33.26778761374 14.4636 14.0145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 42843_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 42843_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 31840_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 31840_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
**** FOUND 16:29:07.79 +34:13:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22485_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 22485_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (27.0") between the two second-epoch detections
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Considering the candidate 18409_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
Preparing report for the candidate 18409_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
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Considering the candidate 19709_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105
The candidate 19709_CrB-02-Q2b1x1_2026-02-27_02-20-49_20.00sec_-15.00C_LIGHT_0105 did not pass the final checks