This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn
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 12.3600 2461083.8600 10.08 14:12:52.98 -38:51:13.7
319.84252 21.32867 galactic Cen Second-epoch detections are separated by 0.4" and 8.9 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 6117207712225235840 | 14:12:53.80 -38:51:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6V 1982MSS...C03....0H HD 124175
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117207712225235840,2461083.8600,10.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117207712225235840 20260212.3600 10.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:12:52.98 -38:51:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 10.48 14:08:18.90 -38:56:20.1
318.90951 21.53586 galactic Cen Second-epoch detections are separated by 1.8" and 8.6 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 6117333159623013504 | 14:08:19.31 -38:56:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117333159623013504,2461083.8600,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117333159623013504 20260212.3600 10.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:18.90 -38:56:20.1 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 10.71 14:09:47.78 -38:54:47.5
319.21190 21.46869 galactic Cen Second-epoch detections are separated by 0.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117148579115646464 | 14:09:48.33 -38:54:54.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117148579115646464,2461083.8600,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117148579115646464 20260212.3600 10.71CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:47.78 -38:54:47.5 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 10.74 14:09:00.90 -38:45:24.3
319.11057 21.66553 galactic Cen Second-epoch detections are separated by 0.7" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117341852645215360 | 14:09:01.31 -38:45:29.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117341852645215360,2461083.8600,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117341852645215360 20260212.3600 10.74CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:00.90 -38:45:24.3 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 10.79 14:10:20.16 -38:48:50.9
319.35306 21.52868 galactic Cen Second-epoch detections are separated by 0.6" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117231729682124032 | 14:10:20.68 -38:48:57.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117231729682124032,2461083.8600,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117231729682124032 20260212.3600 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:20.16 -38:48:50.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 10.96 14:11:51.22 -38:42:08.8
319.69289 21.53785 galactic Cen Second-epoch detections are separated by 0.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117236746204277760 | 14:11:51.84 -38:42:16.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1955AnCap..18.....J CD-38 9150 J-Ks=0.999+/-0.042 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117236746204277760,2461083.8600,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117236746204277760 20260212.3600 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:51.22 -38:42:08.8 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 7.38 13:57:43.12 -31:04:12.6
319.26334 29.69095 galactic Cen Second-epoch detections are separated by 0.2" and 9.7 pix
The object was found in VSX 2" TW Cen
Type: M
# Max. Min./Amp. JD0 Period
6.700 V 13.000 V 2453036.00000 269.800000000000 M4e-M8II:
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TW Cen,2461083.8600,7.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
TW Cen 20260212.3600 7.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:57:43.12 -31:04:12.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_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
RX Cen,2461083.8600,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RX Cen 20260212.3600 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:51:25.45 -36:56:37.7 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 10.76 14:08:37.59 -38:54:49.1
318.97989 21.54073 galactic Cen Second-epoch detections are separated by 1.5" and 8.7 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 6117145899056064512 | 14:08:38.04 -38:54:54.2 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117145899056064512,2461083.8600,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117145899056064512 20260212.3600 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:37.59 -38:54:49.1 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.05 14:10:18.71 -38:42:44.5
319.38361 21.62652 galactic Cen Second-epoch detections are separated by 0.8" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117245473577485312 | 14:10:19.17 -38:42:49.5 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117245473577485312,2461083.8600,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117245473577485312 20260212.3600 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:18.71 -38:42:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.16 14:08:50.18 -38:59:03.8
318.99742 21.46070 galactic Cen Second-epoch detections are separated by 1.2" and 8.7 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 6117144593385979008 | 14:08:50.63 -38:59:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117144593385979008,2461083.8600,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117144593385979008 20260212.3600 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:50.18 -38:59:03.8 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.15 14:08:57.49 -38:48:19.7
319.08261 21.62286 galactic Cen Second-epoch detections are separated by 0.1" and 9.0 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 6117152667925242240 | 14:08:57.85 -38:48:24.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117152667925242240,2461083.8600,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117152667925242240 20260212.3600 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:57.49 -38:48:19.7 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J141132-3849.0,2461083.8600,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J141132-3849.0 20260212.3600 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:33.28 -38:48:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.34 14:10:09.69 -38:52:47.2
319.29574 21.47750 galactic Cen Second-epoch detections are separated by 1.1" and 8.7 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 6117231076847087872 | 14:10:10.32 -38:52:54.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4V 2006A&A...460..695T CD-38 9124
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117231076847087872,2461083.8600,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117231076847087872 20260212.3600 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:09.69 -38:52:47.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.35 14:09:32.42 -38:59:00.1
319.13711 21.41815 galactic Cen Second-epoch detections are separated by 1.9" and 8.6 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 6117146792409226624 | 14:09:32.97 -38:59:06.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117146792409226624,2461083.8600,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117146792409226624 20260212.3600 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:32.42 -38:59:00.1 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.45 14:11:49.16 -38:47:56.8
319.65195 21.44876 galactic Cen Second-epoch detections are separated by 1.0" and 8.7 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 6117187852296516992 | 14:11:49.90 -38:48:05.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117187852296516992,2461083.8600,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117187852296516992 20260212.3600 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:49.16 -38:47:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.46 14:10:31.72 -38:55:12.6
319.35438 21.41622 galactic Cen Second-epoch detections are separated by 1.9" and 8.6 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 6117229874256238080 | 14:10:32.37 -38:55:21.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117229874256238080,2461083.8600,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117229874256238080 20260212.3600 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:31.72 -38:55:12.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.61 14:09:14.33 -38:49:37.8
319.13094 21.58489 galactic Cen Second-epoch detections are separated by 1.3" and 8.7 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 6117153080241400704 | 14:09:14.75 -38:49:43.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117153080241400704,2461083.8600,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117153080241400704 20260212.3600 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:14.33 -38:49:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.73 13:37:36.82 -38:11:45.2
312.82874 23.78687 galactic Cen Second-epoch detections are separated by 1.6" and 9.4 pix
The object was found in VSX 0" V1192 Cen
Type: M
# Max. Min./Amp. JD0 Period
12.000 V < 14.300 V 2453093.00000 305.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1192 Cen,2461083.8600,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
V1192 Cen 20260212.3600 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:37:36.82 -38:11:45.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.67 14:10:39.74 -38:41:51.9
319.45830 21.61821 galactic Cen Second-epoch detections are separated by 0.8" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117245782815922560 | 14:10:40.18 -38:41:57.2 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117245782815922560,2461083.8600,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117245782815922560 20260212.3600 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:39.74 -38:41:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.77 14:11:41.94 -38:48:58.7
319.62209 21.44021 galactic Cen Second-epoch detections are separated by 0.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117187714857555072 | 14:11:42.63 -38:49:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117187714857555072,2461083.8600,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117187714857555072 20260212.3600 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:41.94 -38:48:58.7 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.73 14:09:20.31 -39:00:16.8
319.08988 21.41047 galactic Cen Second-epoch detections are separated by 2.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117146551891054080 | 14:09:20.87 -39:00:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117146551891054080,2461083.8600,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117146551891054080 20260212.3600 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:20.31 -39:00:16.8 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 11.91 14:08:10.31 -38:57:55.9
318.87211 21.51936 galactic Cen Second-epoch detections are separated by 0.9" and 8.9 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 6117331613443084800 | 14:08:10.78 -38:58:01.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117331613443084800,2461083.8600,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117331613443084800 20260212.3600 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:10.31 -38:57:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.26 14:09:20.33 -38:54:56.5
319.12043 21.49478 galactic Cen Second-epoch detections are separated by 0.6" and 8.9 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 6117148098079312768 | 14:09:20.82 -38:55:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117148098079312768,2461083.8600,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117148098079312768 20260212.3600 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:20.33 -38:54:56.5 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.27 14:09:19.16 -38:51:05.5
319.13856 21.55680 galactic Cen Second-epoch detections are separated by 1.7" and 8.7 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 6117152805363487104 | 14:09:19.62 -38:51:10.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117152805363487104,2461083.8600,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117152805363487104 20260212.3600 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:19.16 -38:51:05.5 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.23 14:07:24.71 -39:00:23.2
318.70756 21.52670 galactic Cen Second-epoch detections are separated by 2.0" and 8.7 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 6117311616075348096 | 14:07:25.10 -39:00:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117311616075348096,2461083.8600,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117311616075348096 20260212.3600 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:07:24.71 -39:00:23.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.39 14:09:16.91 -38:57:54.6
319.09219 21.45142 galactic Cen Second-epoch detections are separated by 2.3" and 8.7 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 6117147479604004224 | 14:09:17.43 -38:58:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117147479604004224,2461083.8600,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117147479604004224 20260212.3600 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:16.91 -38:57:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.38 14:08:42.23 -38:55:34.5
318.99094 21.52401 galactic Cen Second-epoch detections are separated by 1.7" and 8.6 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 6117145795976845056 | 14:08:42.73 -38:55:39.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117145795976845056,2461083.8600,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117145795976845056 20260212.3600 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:42.23 -38:55:34.5 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.28 14:12:29.77 -38:40:54.1
319.82747 21.51605 galactic Cen Second-epoch detections are separated by 1.4" and 8.7 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 6117213377281043968 | 14:12:30.47 -38:41:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117213377281043968,2461083.8600,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117213377281043968 20260212.3600 12.28CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:12:29.77 -38:40:54.1 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.43 14:11:04.82 -38:55:27.2
319.46197 21.37757 galactic Cen Second-epoch detections are separated by 1.0" and 9.0 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 6117227812672820736 | 14:11:05.60 -38:55:37.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117227812672820736,2461083.8600,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117227812672820736 20260212.3600 12.43CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:04.82 -38:55:27.2 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.54 14:10:35.37 -38:46:46.9
319.41528 21.54529 galactic Cen Second-epoch detections are separated by 2.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117233104071662976 | 14:10:35.89 -38:46:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117233104071662976,2461083.8600,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117233104071662976 20260212.3600 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:35.37 -38:46:46.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.47 14:10:52.53 -38:50:23.8
319.45092 21.47023 galactic Cen Second-epoch detections are separated by 1.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117232038920567552 | 14:10:53.09 -38:50:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117232038920567552,2461083.8600,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117232038920567552 20260212.3600 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:52.53 -38:50:23.8 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.46 14:09:39.68 -38:55:09.7
319.18305 21.47126 galactic Cen Second-epoch detections are separated by 1.5" and 8.7 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 6117148647835122304 | 14:09:40.13 -38:55:16.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117148647835122304,2461083.8600,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117148647835122304 20260212.3600 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:39.68 -38:55:09.7 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.61 14:09:59.44 -38:59:11.9
319.22502 21.38700 galactic Cen Second-epoch detections are separated by 2.0" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117136377105630720 | 14:09:59.96 -38:59:19.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117136377105630720,2461083.8600,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117136377105630720 20260212.3600 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:59.44 -38:59:11.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.51 14:11:00.24 -38:52:21.3
319.46494 21.43123 galactic Cen Second-epoch detections are separated by 1.7" and 8.6 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 6117228804801844096 | 14:11:00.91 -38:52:29.2 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117228804801844096,2461083.8600,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117228804801844096 20260212.3600 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:00.24 -38:52:21.3 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.51 14:12:41.65 -38:55:47.0
319.77827 21.26926 galactic Cen Second-epoch detections are separated by 0.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117171939434847744 | 14:12:42.52 -38:55:57.5 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117171939434847744,2461083.8600,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117171939434847744 20260212.3600 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:12:41.65 -38:55:47.0 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.52 14:11:40.86 -38:41:36.9
319.66181 21.55729 galactic Cen Second-epoch detections are separated by 1.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117237502118530304 | 14:11:41.45 -38:41:44.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117237502118530304,2461083.8600,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117237502118530304 20260212.3600 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:40.86 -38:41:36.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.63 14:10:24.15 -38:50:43.4
319.35539 21.49492 galactic Cen Second-epoch detections are separated by 1.3" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117231420444474240 | 14:10:24.66 -38:50:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117231420444474240,2461083.8600,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117231420444474240 20260212.3600 12.63CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:24.15 -38:50:43.4 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.79 14:10:01.40 -38:49:14.7
319.28879 21.54205 galactic Cen Second-epoch detections are separated by 1.4" and 8.9 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 6117243205834739584 | 14:10:01.95 -38:49:19.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117243205834739584,2461083.8600,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117243205834739584 20260212.3600 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:01.40 -38:49:14.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.67 14:11:28.34 -38:53:45.8
319.54925 21.37931 galactic Cen Second-epoch detections are separated by 2.4" and 8.5 pix
The object was not found in VSX
The object was found in ASASSN-V13" ASASSN-V J141129.15-385355.1
Type: ROT:
MeanMag 12.43 m Amp. 0.05 m Period 572.6110966 d
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8600,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
VARIABLE_NAME 20260212.3600 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:28.34 -38:53:45.8 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.66 14:12:28.49 -38:43:40.3
319.80682 21.47387 galactic Cen Second-epoch detections are separated by 2.4" and 8.9 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 6117212415206636800 | 14:12:29.31 -38:43:49.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117212415206636800,2461083.8600,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117212415206636800 20260212.3600 12.66CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:12:28.49 -38:43:40.3 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.58 14:11:29.34 -38:51:39.6
319.56486 21.41138 galactic Cen Second-epoch detections are separated by 0.2" and 8.9 pix
The object was found in VSX16" ASAS J141130-3851.8
Type: M
# Max. Min./Amp. JD0 Period
9.774 Ic Y 3.105 Ic 2453204.90000 351.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J141130-3851.8,2461083.8600,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J141130-3851.8 20260212.3600 12.58CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:29.34 -38:51:39.6 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117188711289984000,2461083.8600,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117188711289984000 20260212.3600 12.63CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:12:26.09 -38:45:54.7 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.63 14:08:09.00 -39:01:14.9
318.84911 21.46822 galactic Cen Second-epoch detections are separated by 3.7" and 8.3 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 6117143356435391744 | 14:08:09.57 -39:01:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117143356435391744,2461083.8600,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117143356435391744 20260212.3600 12.63CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:09.00 -39:01:14.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.71 14:11:14.38 -38:47:24.5
319.54043 21.49422 galactic Cen Second-epoch detections are separated by 2.5" and 8.9 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 6117235474894417792 | 14:11:15.07 -38:47:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117235474894417792,2461083.8600,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117235474894417792 20260212.3600 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:14.38 -38:47:24.5 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.86 14:09:20.69 -38:45:04.8
319.17801 21.65018 galactic Cen Second-epoch detections are separated by 0.7" and 8.9 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 6117154450327994624 | 14:09:21.15 -38:45:08.8 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117154450327994624,2461083.8600,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117154450327994624 20260212.3600 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:20.69 -38:45:04.8 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.81 14:08:26.16 -38:57:24.6
318.92744 21.51144 galactic Cen Second-epoch detections are separated by 2.2" and 8.7 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 6117145413716807424 | 14:08:26.51 -38:57:29.5 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117145413716807424,2461083.8600,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117145413716807424 20260212.3600 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:26.16 -38:57:24.6 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.80 14:09:40.95 -38:56:32.3
319.17935 21.44821 galactic Cen Second-epoch detections are separated by 1.6" and 8.6 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 6117148403014045184 | 14:09:41.39 -38:56:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117148403014045184,2461083.8600,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117148403014045184 20260212.3600 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:40.95 -38:56:32.3 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.92 14:08:49.61 -38:51:57.5
319.03588 21.57360 galactic Cen Second-epoch detections are separated by 2.3" and 9.3 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 6117152045146310144 | 14:08:49.95 -38:52:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117152045146310144,2461083.8600,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117152045146310144 20260212.3600 12.92CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:49.61 -38:51:57.5 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 13.06 14:10:35.66 -38:57:31.6
319.35394 21.37555 galactic Cen Second-epoch detections are separated by 2.4" and 9.0 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 6117226816239518080 | 14:10:36.33 -38:57:39.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117226816239518080,2461083.8600,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117226816239518080 20260212.3600 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:35.66 -38:57:31.6 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.92 14:10:38.61 -38:47:26.8
319.42212 21.53140 galactic Cen Second-epoch detections are separated by 0.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117233104071662976 | 14:10:35.89 -38:46:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117233104071662976,2461083.8600,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117233104071662976 20260212.3600 12.92CV 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:38.61 -38:47:26.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3600 2461083.8600 12.88 14:08:38.75 -38:51:49.3
319.00072 21.58692 galactic Cen Second-epoch detections are separated by 2.0" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117339649317806336 | 14:08:39.16 -38:51:53.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117339649317806336,2461083.8600,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 6117339649317806336 20260212.3600 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:38.75 -38:51:49.3 ;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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20_00sec_-15_00C_LIGHT_0398_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: 2461058.93880226 18.01.2026 10:31:42.515 /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
First image: 2461058.93880226 18.01.2026 10:31:42.515 /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
Last image: 2461083.86032744 12.02.2026 08:38:42.291 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 21
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.50
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: 3 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): 5358
Objects passed selection criteria: 5357
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 5188
Average stars matched: 5072 (97.7641 %)
Memory usage VmPeak: 111612 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 Thu Feb 12 02:41:50 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: 2461058.93880226 18.01.2026 10:31:42.515 /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
First image: 2461058.93880226 18.01.2026 10:31:42.515 /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
Last image: 2461083.86032744 12.02.2026 08:38:42.291 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 253
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.23
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: 11 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): 40354
Objects passed selection criteria: 40308
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 39029.2
Average stars matched: 37432 (95.9076 %)
Memory usage VmPeak: 140580 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 Thu Feb 12 02:43:03 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
SExtractor catalog cache: saved Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat to cache
SExtractor catalog cache: saved Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.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: 2461083.85960877
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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits exists and is non-empty
Saving wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits to local_wcs_cache/
'wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits' -> 'local_wcs_cache/wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits'
wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits exists and is non-empty
Saving wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits to local_wcs_cache/
'wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits' -> 'local_wcs_cache/wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits'
wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits exists and is non-empty
Saving wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits to local_wcs_cache/
'wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits' -> 'local_wcs_cache/wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits'
wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
Saving wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits to local_wcs_cache/
'wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits' -> 'local_wcs_cache/wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits'
The image scale is 5.91"/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 13:33:55.586 -34:00:04.95
Second-epoch image center 13:33:54.560 -33:59:52.77
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:33:55.586 -34:00:04.95
Second-epoch image center 13:33:57.214 -34:00:37.79
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:33:54.560 -33:59:52.77
Second-epoch second image center 13:33:57.214 -34:00:37.79
Angular distance between the image centers 0.01551 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits &> /tmp/tmp.ktVV72ppJQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits &> /tmp/tmp.kglxrmmiw0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits &> /tmp/tmp.Qr50Irj5CD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.SzYnABDzOZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
Calibrating the magnitude scale
Found non-empty wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits and wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits and wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat
Found non-empty wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits and wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat
The reference image (wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits) and catalog (wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat) found
'wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.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 4557 out of 5339 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.530505
a=0.000000 b=1.000000 c=22.530505
From vast_summary.log: estimated ref. image limiting mag.: -8.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.03
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
2.2 pix Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
2.1 pix fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
2.1 pix fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
Limiting magnitude estimates:
14.0 mag. Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
14.0 mag. Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
14.0 mag. fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
14.0 mag. fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.1 (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.ktVV72ppJQ (6) ############
Parsing command line arguments...
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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits' -> 'wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
WCS_IMAGE_NAME=wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
WCS-calibrated image found: wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
Checking if the catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits alredy exist and is non-empty...
Catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
WCS catalog name: wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=365, passed=5339
Got 5339 stars (including 4970 good ones) from the SExtractor catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat
util/solve_plate_with_UCAC5 got 5339 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits -region wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.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.kglxrmmiw0 (6) ############
Parsing command line arguments...
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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits' -> 'wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
WCS_IMAGE_NAME=wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
WCS-calibrated image found: wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
Checking if the catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat corresponding to the image wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits alredy exist and is non-empty...
Catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat corresponding to the image wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
WCS catalog name: wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=358, passed=5375
Got 5375 stars (including 5009 good ones) from the SExtractor catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat
util/solve_plate_with_UCAC5 got 5375 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits -region wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.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.Qr50Irj5CD (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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
WCS_IMAGE_NAME=wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
WCS-calibrated image found: wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
Checking if the catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat corresponding to the image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat corresponding to the image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
WCS catalog name: wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=382, passed=5054
Got 5054 stars (including 4667 good ones) from the SExtractor catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat
util/solve_plate_with_UCAC5 got 5054 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.2'
Seting catalog search parameters based on the expected field of view 943.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013100 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010480 (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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 959 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits -region wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.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.SzYnABDzOZ (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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=388, passed=5089
Got 5089 stars (including 4693 good ones) from the SExtractor catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat
util/solve_plate_with_UCAC5 got 5089 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.1'
Seting catalog search parameters based on the expected field of view 943.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013099 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010479 (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 959 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 958 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits'
Saving fully-calibrated image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits'
Preparing the HTML report for the field Cen-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out20335.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out01203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20334.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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: 5s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20319_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 20319_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20322_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 20322_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20325_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 20325_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:03:20.54 -29:06:12.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20327_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 20327_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20328_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 20328_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:25.97 -38:24:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.66, MAG_FAINT_SEARCH_LIMIT=11.64)GAIADR2_OUTPUT=# 2.676 6117278562006045056 212.85902592737 -38.41065473653 10.0283 9.3537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.676#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20329_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 20329_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20330_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 20330_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20332_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 20332_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:32:51.87 -38:07:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.91, MAG_FAINT_SEARCH_LIMIT=11.89)GAIADR2_OUTPUT=# 1.593 6161902756809868544 203.21668587776 -38.12654965709 10.6412 10.2274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20333_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 20333_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:12:24.59 -38:26:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 3.861 6117264680671709184 213.10342345314 -38.44603851764 10.2914 9.7636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20334_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 20334_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20335_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 20335_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:32.08 -38:32:56.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20336_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 20336_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:05:53.43 -37:06:50.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20338_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 20338_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:04:50.56 -35:35:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 2.040 6154978994650061696 196.20997164859 -35.59087716426 10.8556 9.5870 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20339_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 20339_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:03:23.96 -36:24:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 0.655 6120897123486850944 210.85003768312 -36.40569983309 11.3471 10.9040 VARIABLE#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 04141_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 04141_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01203_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 01203_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 20s
Prepared the HTML report for the field Cen-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:51:25.45 -36:56:37.7
13:57:43.12 -31:04:12.6
14:12:52.98 -38:51:13.7
14:08:18.90 -38:56:20.1
14:09:47.78 -38:54:47.5
14:09:00.90 -38:45:24.3
14:10:20.16 -38:48:50.9
14:11:51.22 -38:42:08.8
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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
SExtractor catalog cache: saved Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat to cache
SExtractor catalog cache: saved Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
Creating symlink local_wcs_cache/wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
Creating symlink local_wcs_cache/wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
Creating symlink local_wcs_cache/wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits exists and is non-empty
wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits exists and is non-empty
wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits exists and is non-empty
wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
The image scale is 5.91"/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 13:33:55.586 -34:00:04.95
Second-epoch image center 13:33:54.560 -33:59:52.77
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:33:55.586 -34:00:04.95
Second-epoch image center 13:33:57.214 -34:00:37.79
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:33:54.560 -33:59:52.77
Second-epoch second image center 13:33:57.214 -34:00:37.79
Angular distance between the image centers 0.01551 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/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits &> /tmp/tmp.zpmmOme0T4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits &> /tmp/tmp.ryO7HdrF69
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits &> /tmp/tmp.6kJuIhHyBK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.YZCf4Uhhl7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
Calibrating the magnitude scale
Found non-empty wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits and wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.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_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits and wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat
Found non-empty wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits and wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat
The reference image (wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits) and catalog (wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat) found
'wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.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 8445 out of 39315 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.324195
a=0.000000 b=1.000000 c=22.324195
From vast_summary.log: estimated ref. image limiting mag.: -8.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.09
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 197 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
2.2 pix Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
2.0 pix fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
2.0 pix fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
Limiting magnitude estimates:
14.1 mag. Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
14.1 mag. Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
14.1 mag. fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
14.1 mag. fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zpmmOme0T4 (6) ############
Parsing command line arguments...
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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits' -> 'wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
WCS_IMAGE_NAME=wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
WCS-calibrated image found: wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
Checking if the catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits alredy exist and is non-empty...
Catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits
WCS catalog name: wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1355, passed=39306
Got 39306 stars (including 37887 good ones) from the SExtractor catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat
util/solve_plate_with_UCAC5 got 39306 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits -region wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.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.ryO7HdrF69 (6) ############
Parsing command line arguments...
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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits' -> 'wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
WCS_IMAGE_NAME=wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
WCS-calibrated image found: wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
Checking if the catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat corresponding to the image wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits alredy exist and is non-empty...
Catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat corresponding to the image wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits
WCS catalog name: wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1408, passed=39228
Got 39228 stars (including 37750 good ones) from the SExtractor catalog wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat
util/solve_plate_with_UCAC5 got 39228 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits -region wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cen-02-Q1b1x1_2026-01-18_04-32-17_20.00sec_-14.90C_LIGHT_0508.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.6kJuIhHyBK (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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
WCS_IMAGE_NAME=wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
WCS-calibrated image found: wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
Checking if the catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat corresponding to the image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat corresponding to the image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
WCS catalog name: wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1380, passed=39249
Got 39249 stars (including 37808 good ones) from the SExtractor catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat
util/solve_plate_with_UCAC5 got 39249 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.2'
Seting catalog search parameters based on the expected field of view 943.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013100 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010480 (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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits -region wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.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.YZCf4Uhhl7 (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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.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_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1391, passed=39252
Got 39252 stars (including 37782 good ones) from the SExtractor catalog wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat
util/solve_plate_with_UCAC5 got 39252 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.1'
Seting catalog search parameters based on the expected field of view 943.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013099 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010479 (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 960 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-37-40_20.00sec_-15.00C_LIGHT_0398.fits
Saving fully-calibrated image wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cen-02-Q1b1x1_023930_TTUQ1b1x1_1670_VjneIxIn/wcs_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399.fits
Preparing the HTML report for the field Cen-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out53039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53044.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out53096.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_local.txt__out53176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53241.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 66s
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: 25s
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Considering the candidate 53039_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53039_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:30:28.63 -29:52:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.883 6187948258829064704 202.61947873675 -29.86859397356 13.3120 12.7555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53041_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53041_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:57:04.42 -34:07:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.105 6156094071238980352 194.26825129213 -34.11661412847 13.4947 12.7943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53043_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53043_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:56:04.76 -36:02:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.664 6121811745362210944 209.01905689759 -36.03792116426 13.2849 12.7767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53044_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53044_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:08:33.04 -30:07:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.980 6173072038304910848 212.13706110942 -30.12755712437 13.2939 12.7755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53045_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53045_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:41:48.04 -30:30:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.568 6174966015802999424 205.45093823362 -30.50579718485 13.5943 13.2100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53049_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53049_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:03:39.85 -36:46:57.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)
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Considering the candidate 53054_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53054_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:32:29.93 -37:41:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.829 6162759959267543680 203.12480634799 -37.69928310261 11.7906 11.1747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53055_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53055_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:12:52.98 -38:51:13.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53058_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53058_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:09.05 -38:18:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.30, MAG_FAINT_SEARCH_LIMIT=11.28)GAIADR2_OUTPUT=# 1.495 6117283372369470208 212.78819329068 -38.30372163813 9.7543 9.3468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53059_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53059_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:08:18.91 -38:56:20.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53063_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53063_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:25.96 -38:24:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 2.778 6117278562006045056 212.85902592737 -38.41065473653 10.0283 9.3537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53064_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53064_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:09:47.79 -38:54:47.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53065_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53065_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:09:00.90 -38:45:24.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53066_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53066_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:10:20.16 -38:48:51.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53068_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53068_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53069_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53069_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:10:45.30 -38:21:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 2.056 6117260248265688832 212.68934200399 -38.35286021131 10.2830 9.9212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53070_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53070_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:12:24.58 -38:26:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 3.876 6117264680671709184 213.10342345314 -38.44603851764 10.2914 9.7636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53071_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53071_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:51.23 -38:42:09.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53072_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53072_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:07:24.12 -38:56:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 5.649 6117312097111716480 211.85186835652 -38.93909747109 10.4057 9.7738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53073_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53073_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53074_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53074_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:32.08 -38:32:56.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.08, MAG_FAINT_SEARCH_LIMIT=12.06)
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Considering the candidate 53075_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53075_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:10:00.43 -38:29:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 2.119 6117439326918820864 212.50247305453 -38.48624921089 10.3042 9.3076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53076_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53076_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:10:38.90 -38:25:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 1.904 6117259423631962112 212.66275779894 -38.41829616848 10.5711 10.0816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53078_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53078_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53079_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53079_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53080_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53080_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53081_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53081_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53084_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53084_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53085_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53085_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 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 53086_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53086_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53087_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53087_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53088_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53088_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:14.11 -38:21:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 2.116 6117282616455195904 212.80939486563 -38.36671010317 10.9243 10.6136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53089_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53089_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:44:12.98 -36:32:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 3.696 6163455920063125376 206.05423511328 -36.54881389512 11.4795 10.7762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53091_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53091_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53094_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53094_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53095_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53095_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53096_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53096_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:08:02.77 -38:50:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 5.622 6117337592037629440 212.01301166478 -38.83636765335 11.2486 10.5898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53097_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53097_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53099_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53099_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53102_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53102_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:12:37.90 -38:19:54.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)
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Considering the candidate 53103_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53103_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:10:44.71 -38:39:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 3.949 6117251761410406656 212.68733130947 -38.66554341634 11.2680 10.5492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53104_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53104_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53113_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53113_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:07:35.89 -38:51:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 5.353 6117336904842854016 211.90086211509 -38.86360183408 11.4603 10.7418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53114_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53114_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:06:52.85 -35:29:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53115_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53115_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:38.85 -38:24:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 3.151 6117278733804729984 212.91291990428 -38.41692062259 11.4264 10.8424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53120_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53120_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:12:12.55 -38:21:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 3.199 6117268838200095232 213.05321190117 -38.36490766747 11.7025 11.2810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53121_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53121_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 53123_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53123_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53125_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53125_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:47.98 -38:37:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 5.396 6117238356809099392 212.95134111374 -38.62425402956 11.6122 10.8742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53127_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53127_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:02.64 -38:28:41.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)
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Considering the candidate 53128_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53128_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53129_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53129_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53132_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53132_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:10:45.87 -38:29:12.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)
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Considering the candidate 53139_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53139_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53141_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53141_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53142_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53142_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:12:22.62 -38:28:07.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)
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Considering the candidate 53146_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53146_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53147_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53147_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53148_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53148_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53149_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53149_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:35.21 -38:40:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 5.723 6117237776996451328 212.89786533651 -38.67336383056 12.0667 11.6829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53150_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53150_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53151_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53151_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:45.19 -38:24:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.945 6117278768164470528 212.93913978200 -38.40919903093 11.6772 10.9710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53152_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53152_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53155_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53155_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:54.12 -38:17:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.733 6117281203405091328 212.97603761069 -38.28453743450 11.8987 11.4256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53156_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53156_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53157_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53157_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:12:37.04 -38:15:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 2.776 6117275538349122432 213.15519917957 -38.25394702160 12.0386 11.3684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53158_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53158_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53159_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53159_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:06:47.05 -38:58:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 4.955 6117322748630598144 211.69725185060 -38.98217135353 11.8081 11.1653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53161_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53161_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:12:25.34 -38:03:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.000 6117291103310678144 213.10563213808 -38.05016927000 12.0790 11.3193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53164_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53164_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 53165_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53165_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53166_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53166_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:09:33.39 -38:38:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.850 6117248905248768768 212.38955042256 -38.64441971019 12.0470 11.6848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53167_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53167_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53168_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53168_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53169_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53169_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53170_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53170_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53171_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53171_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:10:08.92 -38:32:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 0.662 6117251276070723840 212.53719916034 -38.54654337149 12.1978 11.6302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53172_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53172_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53173_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53173_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53175_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53175_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:09:57.23 -38:45:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 5.780 6117244442785330688 212.48993346262 -38.75211979370 12.0896 11.4101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53176_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53176_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53178_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53178_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:12:09.40 -38:06:30.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 53181_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53181_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53184_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53184_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:08:42.41 -38:38:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.212 6117346285051536640 212.17773065720 -38.65041073275 12.3993 11.7519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53187_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53187_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53188_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53188_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53190_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53190_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53192_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53192_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:09:33.74 -38:19:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.417 6117450704296065152 212.39071427664 -38.33072431964 12.2315 11.5730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53193_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53193_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:04:29.32 -35:27:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 0.168 6122089750005393664 211.12217212047 -35.45340754294 12.8331 12.0134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53194_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53194_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53196_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53196_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53197_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53197_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:07:56.29 -38:57:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 5.228 6117332502492228864 211.98576950537 -38.95370546260 12.2698 11.7780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53203_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53203_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:07:46.03 -39:01:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.407 6117307733424901632 211.94329427926 -39.02338936975 12.7226 12.2497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53204_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53204_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:12:18.24 -37:14:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 0.942 6117892639249740928 213.07618417041 -37.24344986931 12.3721 11.5229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53205_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53205_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 53206_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53206_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 53212_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53212_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:09:43.75 -38:29:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.964 6117439498717503616 212.43262844893 -38.49062979463 12.3702 11.7735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53222_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53222_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:07:44.35 -38:58:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 5.512 6117332261974060672 211.93585558311 -38.96920497594 12.3061 11.6469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53227_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53227_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53229_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53229_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:16.69 -38:29:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.982 6117254750707320576 212.82051905946 -38.48523384739 12.3425 11.8365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53235_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53235_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53241_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
Preparing report for the candidate 53241_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
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Considering the candidate 53242_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53242_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:06:26.39 -36:50:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.138 6120646774135745280 211.60999408781 -36.83944654203 12.7300 11.8495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53260_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53260_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:07:00.09 -37:44:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.398 6120535654744195328 211.75060441398 -37.73343430582 12.8777 12.4065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53262_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53262_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:50:22.30 -37:42:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 0.405 6115615722461977856 207.59277799791 -37.70100238890 12.9184 12.1537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53264_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53264_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:55:19.60 -38:30:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 0.578 6114588572444013568 208.83174566335 -38.51253700079 13.2082 12.6943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53268_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53268_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:03:39.92 -34:16:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.050 6179303937067826432 195.91645065815 -34.26672485113 13.2176 12.5272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53271_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53271_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:38:47.96 -39:00:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.786 6161643237705645440 204.69970970130 -39.01410963628 13.1038 12.4933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53272_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53272_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:55:37.18 -38:50:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.096 6114511228672892288 208.90484179856 -38.84953447911 12.8889 12.4225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53274_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53274_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:24:52.44 -37:36:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.645 6162588366731750400 201.21858703232 -37.60319573386 13.4116 12.7902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53276_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53276_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:04:56.85 -36:09:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.568 6120883684535682944 211.23702559977 -36.15397365015 13.4494 12.8143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53287_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53287_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:01:25.21 -28:35:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.815 6185319983658210304 195.35486529703 -28.59241823516 13.6010 12.9639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53293_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53293_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:02:30.00 -38:33:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.654 6114402819402413056 210.62550009640 -38.55100866337 12.7395 12.0658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53294_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53294_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:06:51.19 -34:24:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.403 6122251343855157632 211.71285473151 -34.40773160479 13.0941 12.4792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53297_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53297_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:55:47.09 -34:42:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.724 6170082195606954368 208.94662930754 -34.69978031599 13.2419 12.5522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53299_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53299_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:17:47.52 -32:17:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.489 6181263679105075200 199.44855092439 -32.28826673606 13.5806 13.0805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53300_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53300_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:54:27.45 -37:37:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.857 6154461360896040832 193.61455453006 -37.62922558812 13.1681 12.6054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53302_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53302_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:04:16.36 -37:33:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 0.449 6120511293687986816 211.06803982465 -37.56524031238 13.1746 12.7836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53303_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53303_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:57:38.67 -36:04:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.609 6121644275997528448 209.41091169043 -36.08235162439 13.3413 12.7972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53305_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53305_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:06:08.64 -35:59:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.586 6121258136961230464 211.53654047606 -35.99075150708 13.0483 12.2755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53306_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53306_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:03:24.83 -38:09:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.553 6142243214026606464 195.85345644186 -38.15340204068 13.5901 13.0815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53308_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53308_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:00:16.88 -36:46:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.179 6120803149602769664 210.07073112113 -36.76972949852 12.9534 12.2103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53311_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53311_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:54:08.91 -39:04:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.059 6114504214990435840 208.53739282129 -39.07087508214 12.7183 12.0405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53313_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53313_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:56:17.05 -38:07:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.752 6114697664612682240 209.07077354220 -38.13056139507 13.0820 12.4541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53315_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53315_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:04:44.75 -37:58:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.423 6120447182715435136 211.18565952989 -37.97315109832 12.8415 12.3966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53326_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53326_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:07:44.56 -37:39:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.690 6117540928665854976 211.93517203495 -37.65865797215 13.0779 12.6111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53328_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53328_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:08:52.36 -29:48:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.169 6173174361605544320 212.21779519203 -29.81651267730 13.3903 12.7947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53330_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53330_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:58:49.92 -38:27:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.255 6114630555746518528 209.70770174246 -38.46625892973 12.9335 12.4826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53335_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53335_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:56:36.22 -36:48:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.001 6115583321228798336 209.15126356419 -36.80368514889 13.2164 12.2686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53342_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53342_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:20:39.63 -36:46:02.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 53347_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53347_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:07:03.28 -29:34:46.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 53351_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53351_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:07:22.49 -33:29:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.205 6123861338115644032 211.84378492041 -33.48411307110 13.1371 12.4050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53353_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53353_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:51:03.63 -36:29:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.779 6115826240281878400 207.76511286530 -36.49908937435 13.2803 12.4762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53358_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53358_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:58:07.10 -32:14:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.284 6183481462777966208 194.52940888688 -32.23613022883 13.8696 13.6607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53360_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53360_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:08:16.33 -30:39:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.918 6181109266440825344 197.06816837101 -30.65310266410 13.6608 13.1323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53361_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53361_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:53:48.57 -36:27:16.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)
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Considering the candidate 53369_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53369_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:05:39.64 -36:14:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.972 6142871550562170752 196.41495926027 -36.24401014665 13.7672 13.2814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53371_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53371_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:57:33.12 -34:07:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.540 6170123663515235968 209.38841415147 -34.13254987901 13.3233 12.8573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53373_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53373_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:06:47.96 -34:21:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.227 6122252099769211648 211.69977035468 -34.35735339126 13.2059 12.5356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53375_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53375_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:11:12.55 -35:28:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.118 6121195469095079680 212.80227660231 -35.48319188881 12.9303 12.1534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53379_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53379_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:38:48.82 -38:39:38.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)
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Considering the candidate 53382_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53382_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:02:47.95 -29:07:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.892 6173972027227599744 210.70034841348 -29.13130109172 13.1594 12.1438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53386_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53386_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:52:58.27 -37:37:23.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 53388_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53388_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:01:05.75 -38:17:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.353 6142228989094861440 195.27412349618 -38.28492497212 13.5096 13.0320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53391_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53391_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:59:21.97 -36:47:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.368 6154429646856264576 194.84150258607 -36.79329155742 13.6851 13.1492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53395_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53395_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:10:04.97 -35:35:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.388 6121191792603056256 212.52044469348 -35.58931663630 13.2318 12.7070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53397_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53397_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:02:13.28 -32:25:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.509 6170752725901368192 210.55532651089 -32.42202542350 13.4648 12.9341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53400_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53400_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:06:38.72 -33:09:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.692 6124065641120066816 211.66088747144 -33.15504763025 13.3288 12.8167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.692#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53401_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53401_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:59:58.66 -33:53:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.769 6122490590713159936 209.99423504733 -33.88872667254 13.2555 12.5897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53403_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53403_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:00:05.34 -35:18:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.171 6121786834552160384 210.02263271414 -35.31579746702 12.9834 12.2877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53406_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53406_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:59:01.59 -32:27:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.455 6170928785200485760 209.75657672012 -32.46426466565 13.3423 12.5229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53409_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53409_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:54:40.74 -31:28:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.264 6171841139333349888 208.67014855629 -31.47331058069 13.4411 12.9836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53410_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53410_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:00:41.38 -30:41:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.352 6173356231996883840 210.17194084163 -30.69490737043 13.6428 13.3689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53411_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53411_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:58:44.54 -38:09:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.426 6142202012403500672 194.68590936342 -38.16136466649 13.3979 12.8722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53419_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53419_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:22:21.22 -38:22:52.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)
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Considering the candidate 53420_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53420_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:59:52.62 -29:40:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.752 6173577955388153984 209.96979298398 -29.67829745019 13.5541 12.7802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53430_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53430_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:50:48.52 -31:42:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.350 6171914600453944320 207.70234904007 -31.70300487496 13.4374 12.9165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53432_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53432_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:00:12.60 -35:26:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 0.716 6155081180511952256 195.05225803025 -35.43780718081 13.6693 13.2424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53433_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53433_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:59:38.96 -35:53:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.819 6121732271287459584 209.91186066007 -35.89086476661 13.2505 12.5764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53436_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53436_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:58:53.42 -34:42:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.350 6156006179028271488 194.72250577929 -34.71273233051 13.6286 13.1045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53441_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53441_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:55:44.03 -33:46:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.487 6170194655030875904 208.93381975395 -33.76957751186 13.4584 12.9186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53442_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53442_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:22:43.94 -29:13:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 2.103 6182273889772634496 200.68246921663 -29.21796239792 13.5387 13.0213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53445_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53445_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:07:13.53 -33:44:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.290 6179391829278546816 196.80676256540 -33.74657316632 14.0033 13.2988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53454_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53454_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:58:21.88 -37:50:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.605 6154219988029647744 194.59161765838 -37.84220403063 13.4706 13.0359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53456_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53456_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:37:25.35 -38:38:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.866 6161713400291539072 204.35590738017 -38.64420687639 13.4848 13.0710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53459_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53459_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:16:26.56 -33:43:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.075 6167532909178547328 199.11090549185 -33.71834769306 13.9303 13.4570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53460_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53460_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:03:25.73 -34:48:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.844 6155217451234412160 195.85729835095 -34.81329869008 13.8467 13.3469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53463_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53463_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:13:16.85 -33:20:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.595 6179610597732753152 198.32014026057 -33.34194939519 12.2560 10.4245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53464_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53464_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:00:01.36 -35:52:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.238 6155054139397764352 195.00601573368 -35.87316552016 13.2040 12.3049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53465_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53465_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:51:49.87 -38:51:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.568 6114947150673395840 207.95761610074 -38.85858814868 13.1506 12.6219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53467_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53467_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:56:12.54 -36:31:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.753 6154624604012131456 194.05235794234 -36.52850423059 13.6608 12.9020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53469_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53469_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:47:50.35 -31:35:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.749 6171977719293227008 206.95857880306 -31.58545235706 13.7013 13.0608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53471_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53471_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:06:57.72 -38:20:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.364 6142367836797746048 196.74062485392 -38.34561406082 13.5895 13.0544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53473_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53473_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:57:34.25 -38:25:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.108 6142169306229638016 194.39303234059 -38.41993707161 13.2391 12.8143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53475_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53475_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:00:41.14 -36:09:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.260 6121666506748140032 210.17105848726 -36.16077483956 13.0425 12.3857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53476_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53476_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:27:06.71 -32:33:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 0.553 6169058962597948160 201.77777598564 -32.55444340507 14.1446 13.5457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53478_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53478_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:56:38.92 -37:57:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 2.489 6154226271565158656 194.16291032777 -37.96160595223 13.3756 12.8287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53479_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53479_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:32:50.33 -38:58:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.796 6161796001102573184 203.20946374067 -38.96936256250 13.2557 12.6176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53480_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53480_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:07:28.65 -31:36:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 0.893 6180761442809639040 196.86937645613 -31.60825187636 13.8090 13.2879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53481_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53481_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:56:54.81 -29:23:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.198 6173809127707904256 209.22869727052 -29.39723438859 13.5020 12.9668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53484_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53484_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:29:49.59 -35:03:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.945 6167713881920243072 202.45616242233 -35.06550347460 13.1772 12.2423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53490_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53490_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:56:21.84 -36:24:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.701 6154649862716115968 194.09123570345 -36.40281726010 13.5124 13.0371 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53491_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53491_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:07:30.62 -33:33:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.963 6179395746288730880 196.87766270953 -33.55690748800 13.7895 13.1485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53494_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53494_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:02:20.04 -31:24:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.217 6172508714690280192 210.58414553435 -31.40405822118 13.6641 12.9580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53497_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53497_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:08:42.69 -34:52:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.125 6121463268895928960 212.17778734209 -34.87664023208 13.3831 12.6853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53499_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53499_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:03:15.33 -37:19:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 0.357 6142705489946646912 195.81387882114 -37.32065082648 13.5164 13.0046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53501_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53501_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 14:07:52.85 -32:52:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.574 6124094194062382208 211.97051829213 -32.86825994677 13.4938 12.7487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53502_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53502_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:23:49.64 -35:52:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.369 6166128386153288576 200.95691074024 -35.88080785728 13.7606 13.2141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53504_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53504_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 12:57:39.85 -37:43:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.396 6154237064819646080 194.41606329025 -37.71969590040 13.4986 13.0133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53519_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53519_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:33:45.20 -38:55:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 0.290 6161808576766824832 203.43843635668 -38.93092414775 13.1371 12.4809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53522_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53522_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:54:41.82 -37:59:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.684 6115370252195888000 208.67406538940 -37.99512779443 13.0966 12.4782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53526_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53526_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:53:41.28 -37:32:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.822 6115442854323043200 208.42233376149 -37.53334538165 13.3297 12.7941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53528_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 53528_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:44:32.77 -37:52:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.236 6115278786573798016 206.13647835564 -37.87237438956 13.4138 12.8542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31717_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 31717_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:43:56.22 -30:20:40.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26378_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 26378_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:03:20.54 -29:06:12.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07977_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 07977_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:51:25.46 -36:56:38.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34408_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399
The candidate 34408_fd_Cen-02-Q1b1x1_2026-02-12_02-38-42_20.00sec_-14.90C_LIGHT_0399 did not pass the final checks
**** FOUND 13:57:43.12 -31:04:12.4 in the exclusion list exclusion_list_local.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 96s
Prepared the HTML report for the field Cen-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:51:25.45 -36:56:37.7
13:57:43.12 -31:04:12.6
14:12:52.98 -38:51:13.7
14:08:18.90 -38:56:20.1
14:09:47.78 -38:54:47.5
14:09:00.90 -38:45:24.3
14:10:20.16 -38:48:50.9
14:11:51.22 -38:42:08.8
14:08:37.59 -38:54:49.1
14:10:18.71 -38:42:44.5
14:08:50.18 -38:59:03.8
14:08:57.49 -38:48:19.7
14:11:33.28 -38:48:49.9
14:10:09.69 -38:52:47.2
14:09:32.42 -38:59:00.1
14:11:49.16 -38:47:56.8
14:10:31.72 -38:55:12.6
14:09:14.33 -38:49:37.8
13:37:36.82 -38:11:45.2
14:10:39.74 -38:41:51.9
14:11:41.94 -38:48:58.7
14:09:20.31 -39:00:16.8
14:08:10.31 -38:57:55.9
14:09:20.33 -38:54:56.5
14:09:19.16 -38:51:05.5
14:07:24.71 -39:00:23.2
14:09:16.91 -38:57:54.6
14:08:42.23 -38:55:34.5
14:12:29.77 -38:40:54.1
14:11:04.82 -38:55:27.2
14:10:35.37 -38:46:46.9
14:10:52.53 -38:50:23.8
14:09:39.68 -38:55:09.7
14:09:59.44 -38:59:11.9
14:11:00.24 -38:52:21.3
14:12:41.65 -38:55:47.0
14:11:40.86 -38:41:36.9
14:10:24.15 -38:50:43.4
14:10:01.40 -38:49:14.7
14:11:28.34 -38:53:45.8
14:12:28.49 -38:43:40.3
14:11:29.34 -38:51:39.6
14:12:26.09 -38:45:54.7
14:08:09.00 -39:01:14.9
14:11:14.38 -38:47:24.5
14:09:20.69 -38:45:04.8
14:08:26.16 -38:57:24.6
14:09:40.95 -38:56:32.3
14:08:49.61 -38:51:57.5
14:10:35.66 -38:57:31.6
14:10:38.61 -38:47:26.8
14:08:38.75 -38:51:49.3
########### Completed Cen-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
14:12:52.98 -38:51:13.7
14:08:18.90 -38:56:20.1
14:09:47.78 -38:54:47.5
14:09:00.90 -38:45:24.3
14:10:20.16 -38:48:50.9
14:11:51.22 -38:42:08.8
13:57:43.12 -31:04:12.6
13:51:25.45 -36:56:37.7
14:08:37.59 -38:54:49.1
14:10:18.71 -38:42:44.5
14:08:50.18 -38:59:03.8
14:08:57.49 -38:48:19.7
14:11:33.28 -38:48:49.9
14:10:09.69 -38:52:47.2
14:09:32.42 -38:59:00.1
14:11:49.16 -38:47:56.8
14:10:31.72 -38:55:12.6
14:09:14.33 -38:49:37.8
13:37:36.82 -38:11:45.2
14:10:39.74 -38:41:51.9
14:11:41.94 -38:48:58.7
14:09:20.31 -39:00:16.8
14:08:10.31 -38:57:55.9
14:09:20.33 -38:54:56.5
14:09:19.16 -38:51:05.5
14:07:24.71 -39:00:23.2
14:09:16.91 -38:57:54.6
14:08:42.23 -38:55:34.5
14:12:29.77 -38:40:54.1
14:11:04.82 -38:55:27.2
14:10:35.37 -38:46:46.9
14:10:52.53 -38:50:23.8
14:09:39.68 -38:55:09.7
14:09:59.44 -38:59:11.9
14:11:00.24 -38:52:21.3
14:12:41.65 -38:55:47.0
14:11:40.86 -38:41:36.9
14:10:24.15 -38:50:43.4
14:10:01.40 -38:49:14.7
14:11:28.34 -38:53:45.8
14:12:28.49 -38:43:40.3
14:11:29.34 -38:51:39.6
14:12:26.09 -38:45:54.7
14:08:09.00 -39:01:14.9
14:11:14.38 -38:47:24.5
14:09:20.69 -38:45:04.8
14:08:26.16 -38:57:24.6
14:09:40.95 -38:56:32.3
14:08:49.61 -38:51:57.5
14:10:35.66 -38:57:31.6
14:10:38.61 -38:47:26.8
14:08:38.75 -38:51:49.3
###################################################################################
14:12:52.98 -38:51:13.7 -- not an asteroid (will add it to exclusion list)
14:08:18.90 -38:56:20.1 -- not an asteroid (will add it to exclusion list)
14:09:47.78 -38:54:47.5 -- not an asteroid (will add it to exclusion list)
14:09:00.90 -38:45:24.3 -- not an asteroid (will add it to exclusion list)
14:10:20.16 -38:48:50.9 -- not an asteroid (will add it to exclusion list)
14:11:51.22 -38:42:08.8 -- not an asteroid (will add it to exclusion list)
13:57:43.12 -31:04:12.6 -- not an asteroid (will add it to exclusion list)
13:51:25.45 -36:56:37.7 -- not an asteroid (will add it to exclusion list)
14:08:37.59 -38:54:49.1 -- not an asteroid (will add it to exclusion list)
14:10:18.71 -38:42:44.5 -- not an asteroid (will add it to exclusion list)
14:08:50.18 -38:59:03.8 -- not an asteroid (will add it to exclusion list)
14:08:57.49 -38:48:19.7 -- not an asteroid (will add it to exclusion list)
14:11:33.28 -38:48:49.9 -- not an asteroid (will add it to exclusion list)
14:10:09.69 -38:52:47.2 -- not an asteroid (will add it to exclusion list)
14:09:32.42 -38:59:00.1 -- not an asteroid (will add it to exclusion list)
14:11:49.16 -38:47:56.8 -- not an asteroid (will add it to exclusion list)
14:10:31.72 -38:55:12.6 -- not an asteroid (will add it to exclusion list)
14:09:14.33 -38:49:37.8 -- not an asteroid (will add it to exclusion list)
13:37:36.82 -38:11:45.2 -- not an asteroid (will add it to exclusion list)
14:10:39.74 -38:41:51.9 -- not an asteroid (will add it to exclusion list)
14:11:41.94 -38:48:58.7 -- not an asteroid (will add it to exclusion list)
14:09:20.31 -39:00:16.8 -- not an asteroid (will add it to exclusion list)
14:08:10.31 -38:57:55.9 -- not an asteroid (will add it to exclusion list)
14:09:20.33 -38:54:56.5 -- not an asteroid (will add it to exclusion list)
14:09:19.16 -38:51:05.5 -- not an asteroid (will add it to exclusion list)
14:07:24.71 -39:00:23.2 -- not an asteroid (will add it to exclusion list)
14:09:16.91 -38:57:54.6 -- not an asteroid (will add it to exclusion list)
14:08:42.23 -38:55:34.5 -- not an asteroid (will add it to exclusion list)
14:12:29.77 -38:40:54.1 -- not an asteroid (will add it to exclusion list)
14:11:04.82 -38:55:27.2 -- not an asteroid (will add it to exclusion list)
14:10:35.37 -38:46:46.9 -- not an asteroid (will add it to exclusion list)
14:10:52.53 -38:50:23.8 -- not an asteroid (will add it to exclusion list)
14:09:39.68 -38:55:09.7 -- not an asteroid (will add it to exclusion list)
14:09:59.44 -38:59:11.9 -- not an asteroid (will add it to exclusion list)
14:11:00.24 -38:52:21.3 -- not an asteroid (will add it to exclusion list)
14:12:41.65 -38:55:47.0 -- not an asteroid (will add it to exclusion list)
14:11:40.86 -38:41:36.9 -- not an asteroid (will add it to exclusion list)
14:10:24.15 -38:50:43.4 -- not an asteroid (will add it to exclusion list)
14:10:01.40 -38:49:14.7 -- not an asteroid (will add it to exclusion list)
14:11:28.34 -38:53:45.8 -- not an asteroid (will add it to exclusion list)
14:12:28.49 -38:43:40.3 -- not an asteroid (will add it to exclusion list)
14:11:29.34 -38:51:39.6 -- not an asteroid (will add it to exclusion list)
14:12:26.09 -38:45:54.7 -- not an asteroid (will add it to exclusion list)
14:08:09.00 -39:01:14.9 -- not an asteroid (will add it to exclusion list)
14:11:14.38 -38:47:24.5 -- not an asteroid (will add it to exclusion list)
14:09:20.69 -38:45:04.8 -- not an asteroid (will add it to exclusion list)
14:08:26.16 -38:57:24.6 -- not an asteroid (will add it to exclusion list)
14:09:40.95 -38:56:32.3 -- not an asteroid (will add it to exclusion list)
14:08:49.61 -38:51:57.5 -- not an asteroid (will add it to exclusion list)
14:10:35.66 -38:57:31.6 -- not an asteroid (will add it to exclusion list)
14:10:38.61 -38:47:26.8 -- not an asteroid (will add it to exclusion list)
14:08:38.75 -38:51:49.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
13:37:36.82 -38:11:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:51:25.45 -36:56:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:57:43.12 -31:04:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:07:24.71 -39:00:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:09.00 -39:01:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:10.31 -38:57:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:18.90 -38:56:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:26.16 -38:57:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:37.59 -38:54:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:38.75 -38:51:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:42.23 -38:55:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:49.61 -38:51:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:50.18 -38:59:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:08:57.49 -38:48:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:00.90 -38:45:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:14.33 -38:49:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:16.91 -38:57:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:19.16 -38:51:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:20.31 -39:00:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:20.33 -38:54:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:20.69 -38:45:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:32.42 -38:59:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:39.68 -38:55:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:40.95 -38:56:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:47.78 -38:54:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:09:59.44 -38:59:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:01.40 -38:49:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:09.69 -38:52:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:18.71 -38:42:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:20.16 -38:48:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:24.15 -38:50:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:31.72 -38:55:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:35.37 -38:46:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:35.66 -38:57:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:38.61 -38:47:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:39.74 -38:41:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:10:52.53 -38:50:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:11:00.24 -38:52:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:11:04.82 -38:55:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
14:11:14.38 -38:47:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
14:11:28.34 -38:53:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:11:29.34 -38:51:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
14:11:33.28 -38:48:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:11:40.86 -38:41:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
14:11:41.94 -38:48:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:11:49.16 -38:47:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:11:51.22 -38:42:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
14:12:26.09 -38:45:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
14:12:28.49 -38:43:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:12:29.77 -38:40:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
14:12:41.65 -38:55:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
14:12:52.98 -38:51:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
13:37:36.82 -38:11:45.2 -- a known variable star
13:51:25.45 -36:56:37.7 -- a known variable star
13:57:43.12 -31:04:12.6 -- a known variable star
14:07:24.71 -39:00:23.2 -- not a known variable star
14:08:09.00 -39:01:14.9 -- not a known variable star
14:08:10.31 -38:57:55.9 -- not a known variable star
14:08:18.90 -38:56:20.1 -- not a known variable star
14:08:26.16 -38:57:24.6 -- not a known variable star
14:08:37.59 -38:54:49.1 -- not a known variable star
14:08:38.75 -38:51:49.3 -- not a known variable star
14:08:42.23 -38:55:34.5 -- not a known variable star
14:08:49.61 -38:51:57.5 -- not a known variable star
14:08:50.18 -38:59:03.8 -- not a known variable star
14:08:57.49 -38:48:19.7 -- not a known variable star
14:09:00.90 -38:45:24.3 -- not a known variable star
14:09:14.33 -38:49:37.8 -- not a known variable star
14:09:16.91 -38:57:54.6 -- not a known variable star
14:09:19.16 -38:51:05.5 -- not a known variable star
14:09:20.31 -39:00:16.8 -- not a known variable star
14:09:20.33 -38:54:56.5 -- not a known variable star
14:09:20.69 -38:45:04.8 -- not a known variable star
14:09:32.42 -38:59:00.1 -- not a known variable star
14:09:39.68 -38:55:09.7 -- not a known variable star
14:09:40.95 -38:56:32.3 -- not a known variable star
14:09:47.78 -38:54:47.5 -- not a known variable star
14:09:59.44 -38:59:11.9 -- not a known variable star
14:10:01.40 -38:49:14.7 -- not a known variable star
14:10:09.69 -38:52:47.2 -- not a known variable star
14:10:18.71 -38:42:44.5 -- not a known variable star
14:10:20.16 -38:48:50.9 -- not a known variable star
14:10:24.15 -38:50:43.4 -- not a known variable star
14:10:31.72 -38:55:12.6 -- not a known variable star
14:10:35.37 -38:46:46.9 -- not a known variable star
14:10:35.66 -38:57:31.6 -- not a known variable star
14:10:38.61 -38:47:26.8 -- not a known variable star
14:10:39.74 -38:41:51.9 -- not a known variable star
14:10:52.53 -38:50:23.8 -- not a known variable star
14:11:00.24 -38:52:21.3 -- not a known variable star
14:11:04.82 -38:55:27.2 -- not a known variable star
14:11:14.38 -38:47:24.5 -- not a known variable star
14:11:28.34 -38:53:45.8 -- a known variable star
14:11:29.34 -38:51:39.6 -- a known variable star
14:11:33.28 -38:48:49.9 -- a known variable star
14:11:40.86 -38:41:36.9 -- not a known variable star
14:11:41.94 -38:48:58.7 -- not a known variable star
14:11:49.16 -38:47:56.8 -- not a known variable star
14:11:51.22 -38:42:08.8 -- not a known variable star
14:12:26.09 -38:45:54.7 -- a known variable star
14:12:28.49 -38:43:40.3 -- not a known variable star
14:12:29.77 -38:40:54.1 -- not a known variable star
14:12:41.65 -38:55:47.0 -- not a known variable star
14:12:52.98 -38:51:13.7 -- not a known variable star
Found 45 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
52 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 52 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461083.85960877 -observatory 500
22:42:29.78 -08:42:54.0 Mercury (-1.1mag)
22:18:18.68 -12:06:31.3 Venus (-3.9mag)
21:12:15.99 -17:16:49.1 Mars (1.1mag)
07:09:02.98 +22:48:47.4 Jupiter (-2.6mag)
00:01:25.02 -02:11:30.8 Saturn (1.0mag)
03:39:31.53 +19:19:59.5 Uranus (5.7mag)
00:02:29.59 -01:09:31.9 Neptune (7.8mag)
20:27:52.34 -23:02:34.6 Pluto (14.6mag)
17:33:07.48 -28:22:04.5 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 12 02:41 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461083.85960877:
07:08:58.47 +22:48:52.7 Io (5.3mag)
07:09:10.90 +22:48:27.5 Europa (5.5mag)
07:08:51.41 +22:49:01.6 Ganymede (4.9mag)
07:09:05.08 +22:48:30.6 Callisto (6.0mag)
07:11:20.22 +23:09:04.8 Himalia (15.0mag)
07:09:00.05 +22:48:50.0 Thebe (15.8mag)
07:10:57.52 +23:11:52.2 Elara (17.0mag)
07:04:09.12 +24:01:50.0 Pasiphae (17.0mag)
07:18:04.06 +22:33:42.7 Carme (18.0mag)
00:01:20.04 -02:11:10.7 Titan (8.7mag)
00:01:26.82 -02:11:27.8 Rhea (10.1mag)
00:01:00.30 -02:13:14.4 Iapetus (11.5mag)
00:01:27.47 -02:11:16.3 Hyperion (14.7mag)
00:03:30.94 -01:58:06.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 12 02:41 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461083.85960877:
07:40:52.48 +22:58:17.8 JWST
17:00:46.63 +44:32:30.6 Chandra
17:15:41.77 -42:43:05.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 12 02:41 spacecraft.txt
############################################################
Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461083.85960877 at 500
16:40:50.09 -10:51:25.9 17.7mag 10P/Tempel
03:28:59.28 +28:26:11.0 18.1mag 123P/West-Hartley
20:48:17.24 -10:08:57.3 22.4mag 141P/Machholz
00:59:47.23 +09:06:21.1 17.6mag 145P/Shoemaker-Levy 5
11:11:56.00 +29:18:04.0 17.8mag 164P/Christensen
09:38:44.14 -34:07:43.3 18.0mag 195P/Hill
15:51:02.07 -07:25:12.8 18.5mag 210P/Christensen
17:30:41.73 -21:38:34.0 17.4mag 218P/LINEAR
16:04:05.67 -18:17:30.6 15.2mag 235P/LINEAR
03:43:27.55 +25:52:06.3 17.5mag 240P/NEAT
15:02:57.70 +07:29:52.0 14.6mag 24P/Schaumasse
23:54:26.32 +04:19:42.6 18.1mag 261P/Larson
11:27:14.25 -03:35:41.4 17.4mag 29P/Schwassmann-Wachmann 1
01:07:18.10 +01:26:22.2 18.9mag 302P/Lemmon-PanSTARRS
07:06:36.78 +27:17:18.2 19.7mag 407P/PanSTARRS-Fuls
16:49:58.70 -11:18:42.2 17.5mag 40P/Vaisala 1
11:08:07.77 -09:15:49.8 16.6mag 43P/Wolf-Harrington
13:22:51.64 -05:08:22.6 19.4mag 489P/Denning
04:28:05.20 +49:24:17.0 17.7mag 493P/2024 Q2 (LONEOS)
06:02:39.48 +49:16:51.3 17.8mag 63P/Wild 1
22:55:19.69 -03:52:37.5 16.3mag 78P/Gehrels 2
19:24:40.57 -23:28:25.8 15.1mag 88P/Howell
15:22:06.60 -28:11:08.2 18.7mag P/2023 S1 (PanSTARRS)
04:43:15.14 -73:08:54.4 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:39.15 +31:11:09.5 18.1mag C/2017 K2 (PanSTARRS)
20:00:52.01 -64:56:21.8 18.1mag C/2020 V2 (ZTF)
17:17:08.30 +03:22:19.1 16.3mag C/2021 G2 (ATLAS)
22:45:50.36 +28:36:34.0 16.8mag C/2022 E2 (ATLAS)
03:28:23.24 +24:26:38.7 15.7mag C/2022 N2 (PANSTARRS)
09:11:49.76 +28:58:00.6 15.3mag C/2022 QE78 (ATLAS)
08:38:54.23 -07:43:54.8 16.6mag C/2022 R6 (PanSTARRS)
23:40:48.98 +48:06:45.8 17.9mag C/2023 C2 (ATLAS)
10:02:04.75 -22:04:57.3 17.5mag C/2023 F3 (ATLAS)
20:14:13.83 +61:17:12.8 17.2mag C/2023 H5 (Lemmon)
19:32:56.17 -03:17:48.6 16.1mag C/2023 R1 (PANSTARRS)
02:45:58.71 +35:47:06.4 18.5mag C/2023 RS61 (PanSTARRS)
20:43:43.57 +81:15:31.7 18.0mag C/2023 X2 (Lemmon)
06:55:17.95 +63:25:44.3 17.2mag C/2024 A1 (ATLAS)
00:31:41.75 -36:46:25.3 10.8mag C/2024 E1 (Wierzchos)
11:52:19.42 -04:21:47.4 18.1mag C/2024 G2 (ATLAS)
19:18:41.48 +00:21:25.3 19.0mag C/2024 G4 (PanSTARRS)
16:36:59.26 -02:55:59.0 17.8mag C/2024 G6 (ATLAS)
19:46:32.74 +01:32:03.1 15.7mag C/2024 J3 (ATLAS)
02:42:33.27 -33:26:00.6 15.4mag C/2024 T5 (ATLAS)
16:46:13.26 -54:23:38.4 15.3mag C/2025 A6 (Lemmon)
04:55:08.36 +66:11:29.9 16.7mag C/2025 J1 (Borisov)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2025 K1 (ATLAS)
16:01:08.71 -20:07:45.6 15.0mag C/2025 L1 (ATLAS)
02:12:44.68 -17:38:11.7 16.7mag C/2025 Q3 (ATLAS)
01:57:01.63 +16:20:00.7 20.8mag C/2025 R2 (SWAN)
22:17:28.41 +17:32:36.6 16.8mag C/2025 R3 (PANSTARRS)
21:35:19.63 -14:42:18.3 20.4mag C/2025 T1 (ATLAS)
03:30:49.79 -25:06:06.9 17.4mag C/2026 A1 (MAPS)
20:26:13.81 +16:18:04.3 16.6mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.7K Feb 12 02:42 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
18:16:39.86 -19:51:57.30 TCP J06282145-1950371 2026-02-9.38 15.25
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.49 -32:00:30.90 SN 2023kuy 2026-01-21.16 15.43
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
07:40:22.22 -10:00:59.30 AT2025aftz 2025-12-8.46 15.46
18:44:55.93 +47:57:37.60 ASASSN-25ez 2025-12-3.07 15.16
22:41:03.48 +38:58:01.90 ASASSN-25ey 2025-11-26.08 15.68
05:50:46.62 +58:54:53.50 SN 2025aedz 2025-11-24.25 16.66
06:35:50.19 -71:30:42.00 SN 2025adwn 2025-11-24.11 17.58
02:21:35.59 -14:18:04.90 AT2025aeft 2025-11-23.13 16.82
01:42:47.75 +12:31:45.10 AT2025aduf 2025-11-23.15 17.49
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############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:28.44 +41:18:24.5 TCP J00422844+4118245 2025-12-22.8736 18.5mag
16:42:59.22 +26:21:02.0 TCP J16425922+2621020 2025-12-26.8538 13.0mag
08:08:08.72 -19:48:46.5 TCP J08080872-1948465 2025-12-27.7904 16.66Cmag
00:42:58.48 +41:08:11.4 PNV J00425848+4108114 2025-12-28.7654 18.9mag
07:35:31.47 +09:10:34.1 TCP J07353147+0910341 2025-12-29.7527 14.77Cmag
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
-rw-r--r-- 1 apache apache 186K Feb 12 02:41 tocp_transients_list.txt
