This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
OGLE-BLG-LPV-252046,2461128.8683,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
OGLE-BLG-LPV-252046 20260329.3683 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:50:32.23 -19:01:10.7 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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 4123863465516135296,2461128.8683,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4123863465516135296 20260329.3683 13.28CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:45:55.07 -16:39:04.0 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 12.83 18:10:38.31 -16:36:40.7
13.54929 1.18429 galactic Sgr Second-epoch detections are separated by 2.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4145587822368138624 | 18:10:39.37 -16:36:42.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 4145587822368138624,2461128.8683,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4145587822368138624 20260329.3683 12.83CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:10:38.31 -16:36:40.7 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3683* 18 08 25.18 -15 35 35.1 12.3 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 10249,2461128.8683,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 10249 20260329.3683 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:08:25.18 -15:35:35.1 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 12.06 18:10:50.33 -18:33:33.8
11.86551 0.20312 galactic Sgr Second-epoch detections are separated by 4.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J272.6993-18.5538 | 18:10:47.83 -18:33:13.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.6993-18.5538,2461128.8683,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.6993-18.5538 20260329.3683 12.06CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:10:50.33 -18:33:33.8 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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
V4724 Sgr,2461128.8683,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V4724 Sgr 20260329.3683 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:57.31 -18:52:14.9 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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 4095518669864035072,2461128.8683,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095518669864035072 20260329.3683 12.36CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:47.34 -18:51:42.5 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181127.87-182701.8,2461128.8683,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181127.87-182701.8 20260329.3683 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:27.46 -18:27:03.3 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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
VARIABLE_NAME,2461128.8683,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.3683 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:18:20.73 -18:56:03.5 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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
VARIABLE_NAME,2461128.8683,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.3683 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:56:45.80 -16:44:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180748.83-162422.8,2461128.8683,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180748.83-162422.8 20260329.3683 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:48.58 -16:24:23.2 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J172429.02-165842.6,2461128.8683,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J172429.02-165842.6 20260329.3683 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:24:29.05 -16:58:43.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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 J180525-2123.6,2461128.8683,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J180525-2123.6 20260329.3683 12.02CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:05:24.34 -21:23:33.1 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 11.73 18:03:39.34 -22:07:17.6
7.93443 -0.06072 galactic Sgr Second-epoch detections are separated by 0.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J270.9140-22.1217 | 18:03:39.38 -22:07:18.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.672+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J270.9140-22.1217,2461128.8683,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J270.9140-22.1217 20260329.3683 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:03:39.34 -22:07:17.6 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 9.85 18:10:38.70 -19:17:57.4
11.19526 -0.11359 galactic Sgr Second-epoch detections are separated by 0.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J272.6646-19.3047 | 18:10:38.69 -19:17:57.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1922AnHar..97.....C HD 166292 J-Ks=0.112+/-0.030 (A)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.6646-19.3047,2461128.8683,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.6646-19.3047 20260329.3683 9.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:10:38.70 -19:17:57.4 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 11.46 18:12:01.79 -18:47:42.0
11.79481 -0.15754 galactic Sgr Second-epoch detections are separated by 0.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J273.0122-18.7890 | 18:12:01.88 -18:47:42.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.815+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.0122-18.7890,2461128.8683,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.0122-18.7890 20260329.3683 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:12:01.79 -18:47:42.0 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 12.31 18:11:42.79 -18:42:35.5
11.83341 -0.05087 galactic Sgr Second-epoch detections are separated by 1.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J272.9305-18.7064 | 18:11:42.85 -18:42:37.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.766+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.9305-18.7064,2461128.8683,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.9305-18.7064 20260329.3683 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:42.79 -18:42:35.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175202.11-204157.9,2461128.8683,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175202.11-204157.9 20260329.3683 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:52:02.04 -20:41:57.7 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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 J174113-1639.7,2461128.8683,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J174113-1639.7 20260329.3683 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:41:12.50 -16:39:41.6 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 11.89 18:09:17.95 -15:27:52.9
14.39852 2.01955 galactic Ser Second-epoch detections are separated by 0.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4145960316330015232 | 18:09:18.04 -15:27:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.696+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3683* 18 09 17.95 -15 27 52.9 11.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4145960316330015232,2461128.8683,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4145960316330015232 20260329.3683 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:09:17.95 -15:27:52.9 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3683* 18 10 26.62 -15 00 16.2 12.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146072775720222848,2461128.8683,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4146072775720222848 20260329.3683 12.15CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:10:26.62 -15:00:16.2 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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 4095087940490310656,2461128.8683,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095087940490310656 20260329.3683 11.97CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:10:18.93 -19:28:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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 4095533788152801152,2461128.8683,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095533788152801152 20260329.3683 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:10:11.40 -19:02:22.9 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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
V5738 Sgr,2461128.8683,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V5738 Sgr 20260329.3683 10.54CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:03:41.54 -22:10:57.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 11.70 18:09:48.36 -18:56:56.5
11.40624 0.22910 galactic Sgr Second-epoch detections are separated by 0.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4095538293597312000 | 18:09:48.48 -18:56:56.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.717+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095538293597312000,2461128.8683,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095538293597312000 20260329.3683 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:09:48.36 -18:56:56.5 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 10.66 18:12:00.19 -18:04:25.1
12.42430 0.19480 galactic Sgr Second-epoch detections are separated by 0.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4095698306894619648 | 18:12:00.51 -18:04:24.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095698306894619648,2461128.8683,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095698306894619648 20260329.3683 10.66CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:12:00.19 -18:04:25.1 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.3683* 17 57 09.27 -15 34 53.7 12.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175709.80-153448.6,2461128.8683,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175709.80-153448.6 20260329.3683 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:57:09.27 -15:34:53.7 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 12.59 18:05:08.88 -20:59:02.6
9.09583 0.19515 galactic Sgr Second-epoch detections are separated by 1.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J271.2897-20.9885 | 18:05:09.01 -20:59:03.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.785+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J271.2897-20.9885,2461128.8683,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J271.2897-20.9885 20260329.3683 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:05:08.88 -20:59:02.6 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 11.80 18:11:53.28 -18:59:57.2
11.59962 -0.22632 galactic Sgr Second-epoch detections are separated by 1.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J272.9744-18.9982 | 18:11:53.19 -19:00:00.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.9744-18.9982,2461128.8683,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.9744-18.9982 20260329.3683 11.80CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:53.28 -18:59:57.2 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 11.93 18:11:36.98 -19:03:05.7
11.52282 -0.19522 galactic Sgr Second-epoch detections are separated by 1.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4095489605845236352 | 18:11:37.09 -19:03:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.756+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095489605845236352,2461128.8683,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095489605845236352 20260329.3683 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:36.98 -19:03:05.7 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 11.14 18:11:11.91 -17:05:28.3
13.19329 0.83565 galactic Sgr Second-epoch detections are separated by 0.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4096021730790844928 | 18:11:11.96 -17:05:25.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4096021730790844928,2461128.8683,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4096021730790844928 20260329.3683 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:11.91 -17:05:28.3 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173337.06-171726.7,2461128.8683,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173337.06-171726.7 20260329.3683 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:33:36.97 -17:17:26.8 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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 4069559032829939200,2461128.8683,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4069559032829939200 20260329.3683 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:00:22.36 -22:12:21.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3683 2461128.8683 12.48 18:11:06.80 -16:59:49.4
13.26599 0.89883 galactic Sgr Second-epoch detections are separated by 4.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J272.7848-16.9879 | 18:11:08.37 -16:59:16.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.571+/- (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.7848-16.9879,2461128.8683,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.7848-16.9879 20260329.3683 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:11:06.80 -16:59:49.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20_00sec_-14_90C_LIGHT_0324_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20_00sec_-14_90C_LIGHT_0323_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: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
First image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Last image: 2461128.86857324 29.03.2026 08:50:34.728 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.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.: -8.23
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: 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): 10151
Objects passed selection criteria: 10129
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 8411
Average stars matched: 8180.75 (97.2625 %)
Memory usage VmPeak: 117364 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 03:52:43 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
First image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Last image: 2461128.86857324 29.03.2026 08:50:34.728 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 446
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
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: 40 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): 135152
Objects passed selection criteria: 134847
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 108594
Average stars matched: 103608 (95.409 %)
Memory usage VmPeak: 1974984 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 03:56:09 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat to cache
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461128.86805459
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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits exists and is non-empty
Saving wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits to local_wcs_cache/
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits exists and is non-empty
Saving wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits to local_wcs_cache/
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits exists and is non-empty
Saving wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits to local_wcs_cache/
'wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits' -> 'local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits'
wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits exists and is non-empty
Saving wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits to local_wcs_cache/
'wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits' -> 'local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:59.843 -18:02:34.77
Angular distance between the image centers 0.17 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 17:46:18.174 -18:00:45.70
Second-epoch image center 17:47:01.209 -18:02:37.28
Angular distance between the image centers 0.17 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 17:46:59.843 -18:02:34.77
Second-epoch second image center 17:47:01.209 -18:02:37.28
Angular distance between the image centers 0.00546 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits &> /tmp/tmp.zbwIb86gcB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits &> /tmp/tmp.cNly6w0Riy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits &> /tmp/tmp.f89xhIf7rd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits &> /tmp/tmp.jLQcqlbVw8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
The reference image (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits) and catalog (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat) found
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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 10414 out of 15752 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.846952
a=0.000000 b=1.000000 c=22.846952
From vast_summary.log: estimated ref. image limiting mag.: -8.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
2.3 pix Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
2.8 pix fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
2.8 pix fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
Limiting magnitude estimates:
14.6 mag. Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
14.6 mag. Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
13.8 mag. fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
13.8 mag. fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
All-image limiting magnitude estimate: 13.8 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zbwIb86gcB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1456, passed=15752
Got 15752 stars (including 14271 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 15752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 919 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 918 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: 0.41"
Excluding outliers - 914 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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.cNly6w0Riy (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1474, passed=15602
Got 15602 stars (including 14101 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 15602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 919 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 918 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: 0.43"
Excluding outliers - 915 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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.f89xhIf7rd (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=463, passed=7819
Got 7819 stars (including 7350 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat
util/solve_plate_with_UCAC5 got 7819 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 921 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: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.84"
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 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.85"
Estimated accuracy of the plate solution: 0.99"
Excluding outliers - 916 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.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.jLQcqlbVw8 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=469, passed=7811
Got 7811 stars (including 7338 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat
util/solve_plate_with_UCAC5 got 7811 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 918 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: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.86"
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 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.88"
Estimated accuracy of the plate solution: 1.01"
Excluding outliers - 913 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
Saving fully-calibrated image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits'
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits'
Preparing the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20827.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20749_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 20749_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:03:48.57 -22:13:45.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20751_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 20751_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:41.36 -16:04:43.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20752_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 20752_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:14.83 -19:25:57.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20827_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 20827_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20877_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 20877_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:44:05.59 -15:12:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 2.481 4148982770717313024 266.02354154694 -15.20086779790 11.4617 10.6424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01611_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 01611_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:03:49.24 -22:14:15.4 in the exclusion list exclusion_list_tycho2.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
17:50:32.23 -19:01:10.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat to cache
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Creating symlink local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits exists and is non-empty
wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits exists and is non-empty
wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits exists and is non-empty
wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:59.843 -18:02:34.77
Angular distance between the image centers 0.17 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 17:46:18.174 -18:00:45.70
Second-epoch image center 17:47:01.209 -18:02:37.28
Angular distance between the image centers 0.17 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 17:46:59.843 -18:02:34.77
Second-epoch second image center 17:47:01.209 -18:02:37.28
Angular distance between the image centers 0.00546 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits &> /tmp/tmp.3gwxe7OGnX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits &> /tmp/tmp.3mguVPmwOB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits &> /tmp/tmp.cGKNimxkjs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits &> /tmp/tmp.75hbJ0CQs7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
The reference image (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits) and catalog (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat) found
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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 12785 out of 179796 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.613163
a=0.000000 b=1.000000 c=22.613163
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.74
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.74
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 250 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
1.9 pix Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
2.5 pix fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
2.4 pix fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
Limiting magnitude estimates:
14.7 mag. Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
14.7 mag. Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
13.9 mag. fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
13.9 mag. fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
All-image limiting magnitude estimate: 13.9 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.3gwxe7OGnX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=17851, passed=179768
Got 179768 stars (including 161620 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 179768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 923 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: 0.41"
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 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 919 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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.3mguVPmwOB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=17987, passed=181054
Got 181054 stars (including 162799 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 181054 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 925 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: 0.45"
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 924 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: 0.48"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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.cGKNimxkjs (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=4829, passed=73401
Got 73401 stars (including 68508 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat
util/solve_plate_with_UCAC5 got 73401 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 927 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: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.71"
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 920 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.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.75hbJ0CQs7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=4975, passed=75656
Got 75656 stars (including 70599 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat
util/solve_plate_with_UCAC5 got 75656 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 924 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: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.72"
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 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 917 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Saving fully-calibrated image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-49-49_20.00sec_-14.90C_LIGHT_0323.fits
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sgr-01-Q2b1x1_035117_TTUQ2b1x1_9945_vFukTLhN/wcs_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324.fits
Preparing the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out14264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out206979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208956.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209114.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out42670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out46826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out73851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out208374.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out53174.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out104400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99402.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 44s
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: 16s
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Considering the candidate 208310_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208310_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 208322_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208322_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:41:17.55 -16:55:17.5 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 208325_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208325_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:50:09.11 -15:51:11.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208328_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208328_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:59.98 -18:07:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.400 4095697134347656192 273.00081200188 -18.12120110165 12.2435 10.9267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208336_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208336_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:03:03.49 -15:15:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208337_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208337_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:24:05.39 -15:08:45.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)
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Considering the candidate 208339_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208339_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:00:04.95 -15:56:46.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208344_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 208344_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 208345_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208345_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:37.24 -16:32:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 4.066 4145589432956778624 272.65619596117 -16.53378354590 12.3376 11.1364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208347_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208347_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:00:16.26 -16:16:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208348_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208348_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:37.15 -18:27:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.177 4095591478151582336 272.65512717163 -18.45388026375 12.4353 11.8230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208350_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208350_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:49:43.66 -15:52:05.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 208352_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208352_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:58:34.06 -18:18:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.911 4143635394636851200 269.64187795855 -18.31160941976 12.8733 11.7529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208358_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208358_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:09:16.16 -15:27:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.807 4145960311973441792 272.31765950940 -15.46277528109 12.4852 11.2505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208368_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208368_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:59.45 -15:40:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208373_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 208373_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208374_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208374_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:18:28.86 -17:33:20.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 208375_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208375_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:03.48 -19:20:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 3.851 4094712934013849088 273.01336692427 -19.33966074357 12.7205 12.3938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208376_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208376_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:16.20 -18:05:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208377_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208377_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:06:21.64 -15:03:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208379_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208379_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:10.29 -19:23:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.753 4095100992880956544 272.54283395975 -19.39648531024 12.2299 11.8022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208381_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208381_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:43:15.86 -18:46:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.292 4120196143193790976 265.81553892723 -18.78026520223 12.9521 12.4180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208382_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208382_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208387_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208387_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:05.84 -16:36:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 4.401 4145590193189935360 272.77554969185 -16.60368717595 12.3384 11.2729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208389_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208389_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:49.76 -13:46:49.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208396_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208396_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208401_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208401_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:09:07.97 -19:20:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208402_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208402_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:59:48.07 -20:13:19.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208404_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208404_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:01:12.78 -15:19:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.694 4145459110823234816 270.30372669984 -15.33181570902 12.6305 12.0736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208406_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208406_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:19.34 -16:38:29.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)
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Considering the candidate 208409_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208409_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:07:12.80 -15:56:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.264 4145916262792515584 271.80334718348 -15.94048333775 12.6182 11.8610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208410_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208410_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:04:31.14 -21:36:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.930 4070060062236710656 271.12998208155 -21.60874691286 12.0201 11.3776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208414_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208414_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:04:56.14 -21:31:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.878 4070066624946737280 271.23473931881 -21.52440814745 12.1939 11.8226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208415_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208415_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:55.59 -15:42:27.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)
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Considering the candidate 208417_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208417_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:33.92 -19:15:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208420_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208420_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:09.64 -17:05:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.742 4096021941253062144 272.79022377843 -17.08868481407 11.9892 10.9226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208421_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208421_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:19:13.02 -20:42:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 2.028 4115929522684926976 259.80474799415 -20.70418340822 12.7569 11.9149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208423_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208423_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:56:00.97 -13:48:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208424_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 208424_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 208425_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208425_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:18:11.68 -19:50:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.132 4122214266757245568 259.54898320775 -19.84987921145 12.5279 11.7076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208426_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208426_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:06:50.81 -14:10:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208427_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208427_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 208428_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208428_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:06:13.06 -19:49:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208429_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208429_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:07:46.97 -18:52:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.070 4095366013856273280 271.94622588917 -18.87197628666 12.3983 11.8416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208430_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208430_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:38:12.55 -16:06:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 1.528 4124849173329895680 264.55264293249 -16.11361846608 12.3245 11.4436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208433_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208433_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:20:34.60 -20:44:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.342 4115914747999276928 260.14385218627 -20.73681256084 12.3488 11.4226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208436_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208436_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:07:15.00 -19:31:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.421 4095116665232459776 271.81321312324 -19.53128161815 11.6242 10.7430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208439_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 208439_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 208446_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208446_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:31.07 -18:24:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208449_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208449_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:17:34.71 -21:43:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208450_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208450_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:17:59.77 -21:57:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208451_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208451_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:05:19.11 -14:19:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208453_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208453_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:03:48.59 -22:13:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208454_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208454_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:41.37 -16:04:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208457_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208457_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:51.01 -15:40:46.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 208470_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208470_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:29.49 -19:19:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.34, MAG_FAINT_SEARCH_LIMIT=10.32)GAIADR2_OUTPUT=# 2.975 4095464351436703616 272.87371573828 -19.32729688798 8.5554 7.3779 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208485_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208485_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:50.48 -19:43:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.74, MAG_FAINT_SEARCH_LIMIT=10.72)GAIADR2_OUTPUT=# 1.229 4094316461281987200 272.96019435209 -19.72131546349 9.2110 8.6886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208513_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208513_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:13.51 -19:54:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.41, MAG_FAINT_SEARCH_LIMIT=11.39)GAIADR2_OUTPUT=# 1.483 4094306531317552384 272.80587445770 -19.91576503907 9.9631 9.8012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208520_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208520_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:46.68 -19:33:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.48, MAG_FAINT_SEARCH_LIMIT=11.46)GAIADR2_OUTPUT=# 3.759 4095083366335181056 272.69559281756 -19.56135520803 9.6010 8.4229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208532_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208532_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:50:32.24 -19:01:10.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 208558_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208558_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:07.58 -19:54:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 0.910 4094306771835740544 272.78185189224 -19.91303692003 10.2799 9.5120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208559_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208559_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:25.19 -19:02:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.91, MAG_FAINT_SEARCH_LIMIT=11.89)GAIADR2_OUTPUT=# 2.434 4095488364574148736 272.85567297270 -19.03744717591 9.9233 8.5562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208580_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208580_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:33.11 -19:30:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 1.278 4094709154426813440 272.88807693965 -19.50875357276 10.5978 10.0507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208581_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 208581_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 208588_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208588_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:02.00 -19:25:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 2.760 4094711289051104512 273.00895342555 -19.42205147759 10.4459 9.4345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208602_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208602_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:37:26.68 -15:24:56.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 208609_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208609_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:27.01 -19:54:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 0.845 4094304023056618240 272.86241870161 -19.91009316217 10.8417 10.4600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208617_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208617_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:06:21.40 -19:58:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 1.629 4094959435073683072 271.58964576931 -19.97159289191 10.8794 10.2489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208621_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208621_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:12.98 -19:35:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 0.583 4094693215828561920 273.05424752905 -19.58999206777 10.7448 10.0675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208635_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208635_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:45.51 -19:36:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 3.683 4094329449263184000 272.94069048992 -19.61180166448 10.4535 9.3027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208647_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208647_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:56.91 -19:00:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 3.899 4095478473289988224 272.98826857904 -19.00516069220 10.3262 8.9962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208660_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208660_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:05.01 -19:41:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 3.742 4094316255123530240 273.02197235150 -19.69538477232 10.7286 9.6519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208666_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208666_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:04:48.47 -22:02:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 4.881 4069892700266657280 271.20339272755 -22.05007186199 10.3306 8.8976 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208678_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208678_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:29.65 -18:48:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 3.338 4095520082935241856 272.87449291640 -18.80213969516 10.6862 9.4961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208693_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208693_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:01.39 -19:52:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 0.984 4094309451895195648 273.00597795752 -19.88207102387 11.0119 10.2792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208697_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208697_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:13.26 -19:09:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208715_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208715_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:43.24 -19:45:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 0.376 4094314842067505152 272.93013406257 -19.75101636248 10.9970 10.5044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208729_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208729_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:06.44 -19:51:19.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 208738_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208738_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:26.43 -19:39:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 1.290 4094329517982682240 272.86049062270 -19.65523419083 11.3397 10.5093 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 208741_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208741_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:25.45 -19:36:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 3.519 4094330033378796288 272.85707927801 -19.60529107574 11.4462 10.8458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208748_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208748_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:35.46 -19:49:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 3.660 4094313334545753344 272.89881503497 -19.82642303527 11.3884 10.5935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208768_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208768_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:24.22 -19:04:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.766 4095488162735735168 272.85172935823 -19.07395155265 11.0654 9.9396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208781_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208781_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:38.97 -13:54:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208795_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208795_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:01.20 -19:05:07.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)
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Considering the candidate 208800_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208800_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:15.18 -19:04:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.797 4095487819138380416 272.81392307570 -19.08233174746 11.2717 9.9742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208812_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208812_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:47.45 -15:11:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208815_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208815_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:25:59.49 -14:03:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208822_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208822_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:52.80 -19:38:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.570 4094329101358925056 272.96992007421 -19.63888925256 11.5175 10.9904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208836_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208836_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:09.43 -19:51:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.115 4094309585029149440 273.03904636644 -19.86012318723 11.6631 11.2436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208843_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208843_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:37.28 -19:24:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 1.880 4094710941133207424 272.90588578950 -19.41020284295 11.4735 10.6860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208846_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208846_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:19:52.33 -17:46:29.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 208847_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208847_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:02.38 -19:10:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 4.725 4095471601342213760 273.01117803390 -19.18236555176 11.2095 10.0872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208859_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208859_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:36.66 -19:29:34.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)
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Considering the candidate 208869_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208869_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:29:59.56 -17:21:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208880_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208880_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:48.12 -19:21:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.233 4094712659120124928 272.95106246654 -19.35995667148 11.5240 10.7038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208886_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208886_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:48.95 -19:47:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 2.932 4094320855021721088 272.70481839821 -19.79626894898 11.5082 10.5274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208891_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208891_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:10.08 -19:05:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.579 4095476888420195840 273.04242656834 -19.09000639131 11.5807 10.5328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208916_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208916_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:56.65 -19:07:33.3 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 208927_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208927_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:44.21 -19:46:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.928 4094321134206548352 272.68507137777 -19.77515222877 11.7347 10.8635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208948_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208948_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:56.80 -19:32:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.774 4094705722773400064 272.98668139805 -19.54942422170 11.8524 11.4554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208955_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 208955_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 208956_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208956_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:54.56 -19:32:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 3.798 4095084882473412864 272.72845164237 -19.53921149816 11.6039 10.4161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208964_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208964_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:20.04 -19:15:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.822 4095467748729799680 272.83462040946 -19.25726888981 11.3248 10.0607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208967_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208967_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:03.55 -19:13:28.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)
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Considering the candidate 208992_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208992_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:57.31 -19:53:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.142 4094306114693236864 272.73903547889 -19.89694162346 11.8491 11.2157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208993_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208993_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:25.48 -18:54:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.898 4095494862885335680 272.85701627008 -18.90345840228 11.9210 11.0318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208996_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 208996_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:37:09.42 -20:30:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209000_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209000_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:34.92 -19:51:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 4.852 4094313025308084736 272.89693139315 -19.85866074436 11.0450 9.5742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209001_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209001_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 209006_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209006_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:14.65 -19:55:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 5.432 4094306428238321280 272.81245065728 -19.93116605503 11.8982 10.7362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209008_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209008_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:59.38 -19:56:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.923 4094261687553864960 272.99703294939 -19.93969935967 12.0210 11.7355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209010_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209010_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:23:37.60 -16:00:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209012_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209012_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:57.09 -19:11:53.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)
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Considering the candidate 209023_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209023_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:59.28 -19:36:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.562 4094704481502396288 272.99746062026 -19.61536151546 11.7133 10.7509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209029_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209029_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:54.75 -19:49:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.241 4094310581459222784 272.97825385229 -19.82207259095 11.9349 11.2882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209039_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209039_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:59:25.84 -15:09:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.241 4145502919491958144 269.85768580369 -15.15379665701 12.6364 11.8940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209041_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209041_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:00.43 -19:35:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 4.499 4094704584581643520 273.00310197054 -19.59744463471 11.8384 10.5336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209047_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209047_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:43.32 -14:29:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.419 4146500863692782208 272.93090616171 -14.49227802388 12.4246 11.5782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209050_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209050_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:41.31 -19:17:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 0.842 4095464896871516288 272.92219427050 -19.29186338781 12.1658 11.4067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209051_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209051_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:32.35 -19:52:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.524 4094307111125649280 272.88461819141 -19.87466839176 12.1256 11.8626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209054_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209054_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:35:38.50 -14:39:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 0.985 4137299909884254976 263.91024251705 -14.65743790029 12.7497 12.2888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209055_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209055_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:25.28 -18:50:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.822 4095519288339379072 272.85615210937 -18.84659119961 11.7493 10.3076 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#
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Considering the candidate 209070_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209070_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:48.53 -19:44:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.508 4094321645295701120 272.70353395554 -19.73344935174 12.0337 11.1240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209095_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209095_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:31.56 -18:57:57.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 209103_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209103_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:56:25.74 -16:13:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209111_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209111_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:55.88 -19:13:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.791 4095468955641928064 272.73422993502 -19.22832059536 11.4241 9.9788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209114_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209114_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:35:51.64 -15:50:49.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)
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Considering the candidate 209129_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209129_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:21.02 -19:50:29.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 209150_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209150_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:09.27 -19:00:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 5.699 4095501700473958784 273.04028093014 -19.00790406334 11.0501 9.5613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209152_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209152_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:34.82 -19:54:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.596 4094303984389458176 272.89608379393 -19.90902529711 12.3125 11.4735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209153_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209153_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:47.02 -19:31:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 2.447 4094706062050360448 272.94662319688 -19.52546929428 11.8802 10.6625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209157_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209157_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:23:35.80 -16:43:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209162_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209162_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:08.92 -18:49:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209172_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209172_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:10.84 -19:33:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.890 4094705134337482496 273.04571763838 -19.55947747655 12.2290 11.3630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209176_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209176_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:43:19.93 -14:59:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.805 4149049252456462208 265.83288947914 -14.98510930963 12.6427 11.6011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209177_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209177_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:03.81 -19:39:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 3.823 4094331162943588736 272.76629276558 -19.65715313553 12.4230 11.5238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209181_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209181_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:38:01.00 -15:21:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.404 4125171540725984640 264.50328113737 -15.36265646014 12.9751 12.0429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209187_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209187_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:53.49 -16:03:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209196_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209196_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:50.49 -19:26:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.511 4095086836670072064 272.71135166333 -19.43412382829 12.1577 11.0811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209199_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209199_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:54.70 -19:34:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.232 4094704863779924096 272.97811083063 -19.57973379344 12.0227 11.1725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209201_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 209201_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 209207_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209207_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:21:38.35 -14:37:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.948 4137898933242348544 260.40917405393 -14.62676535999 13.1508 12.2673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209216_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209216_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:35:14.51 -14:20:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 0.781 4137368281443572992 263.81059229670 -14.34427047217 13.1201 11.4187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209219_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209219_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:02.15 -19:28:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209227_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209227_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:05.79 -19:55:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 4.739 4094261859352522368 273.02551921487 -19.91973087811 11.9792 10.7073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209238_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209238_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:02:54.11 -14:31:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209263_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209263_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:25:14.55 -18:35:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209266_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209266_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:58.92 -19:50:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209281_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209281_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:34:15.73 -19:06:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209282_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209282_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:29:28.93 -17:46:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.950 4122757627338248320 262.36940773516 -17.77258350034 13.2743 12.3705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209283_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209283_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:13.72 -19:39:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209285_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209285_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:41:30.62 -16:24:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209291_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209291_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:56.18 -16:32:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209293_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209293_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 209323_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209323_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:44:22.87 -17:08:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.432 4123824467221273216 266.09498851590 -17.14652262713 13.5088 12.6989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209327_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 209327_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 209329_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209329_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:29:32.87 -20:22:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209336_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209336_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:28:22.94 -15:40:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209337_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209337_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:40:16.29 -15:05:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209341_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209341_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:34:56.85 -15:44:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209345_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209345_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:20:56.58 -19:10:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209365_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209365_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:54:56.00 -15:21:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.379 4148394738153278720 268.73353371847 -15.35244699265 12.1901 10.3053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209369_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209369_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:26:31.99 -15:08:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209382_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 209382_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:49:45.19 -17:43:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209383_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 209383_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 25679_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 25679_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:19:58.07 -21:11:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195040_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 195040_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:43:29.49 -14:52:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90291_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 90291_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:29:56.34 -17:40:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119291_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 119291_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 104635_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 104635_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 60437_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 60437_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:38:29.57 -19:05:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168596_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 168596_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:06:52.39 -14:10:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197668_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 197668_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:19:42.29 -14:55:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.185 4137782148795895808 259.92598734580 -14.91961061893 13.7705 11.8868 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129825_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 129825_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:44.24 -14:11:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190967_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 190967_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:31:56.02 -19:19:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191506_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 191506_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:18:14.74 -21:44:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192007_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 192007_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:11.59 -19:29:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136842_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 136842_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:02:00.58 -15:16:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192685_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 192685_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:09:31.49 -19:17:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.717 4095106353000135936 272.38131935646 -19.29022502177 11.7963 11.1237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 25354_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 25354_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 44480_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 44480_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:21:49.44 -19:58:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15441_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 15441_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 57309_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 57309_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:09:51.68 -19:16:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56928_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 56928_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 111310_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 111310_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:48:11.39 -16:47:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66281_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 66281_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 68019_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 68019_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 36079_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 36079_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 113772_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 113772_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 194022_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 194022_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:08:24.12 -15:02:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140816_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 140816_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 193616_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 193616_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:19:10.83 -15:06:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193265_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 193265_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:38.57 -19:20:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.055 4095463316323553408 272.91017055463 -19.34781703827 11.7949 11.6057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 179667_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 179667_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 192686_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 192686_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:09:12.28 -14:59:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.526 4146081915437136256 272.30232235604 -14.99644949657 12.4632 11.2469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 178698_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 178698_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:44:10.67 -14:56:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21013_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 21013_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:28:53.05 -21:36:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53945_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 53945_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 192189_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 192189_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:34.08 -17:12:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192011_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 192011_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:39.85 -19:22:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191765_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 191765_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:56:09.53 -20:47:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191748_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 191748_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:02.05 -19:19:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 2.661 4095465927663668480 272.75928400146 -19.32870866417 9.7678 8.7944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191720_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 191720_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:08:46.09 -16:26:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 5.302 4144151619667384704 272.19343974441 -16.43319686444 11.5054 10.3029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191701_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 191701_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:02:38.61 -22:12:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120701_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 120701_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:42:00.34 -16:20:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135786_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 135786_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:09:52.72 -15:12:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56322_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 56322_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:09:09.59 -19:20:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61514_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 61514_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 85879_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 85879_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:04:15.10 -17:56:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73851_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 73851_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:44.96 -18:26:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.229 4095583266173046272 272.93747479498 -18.44089734681 11.9164 11.5111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191168_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 191168_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:28:44.15 -20:57:39.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 84473_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 84473_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:21.19 -17:58:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59063_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 59063_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:57.52 -19:10:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55937_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 55937_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:33.72 -19:21:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197834_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 197834_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:56:17.12 -16:53:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57104_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 57104_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:26.31 -19:16:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14743_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 14743_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
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Considering the candidate 14264_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 14264_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:05:18.11 -22:11:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.167 4069702450400374528 271.32640627064 -22.19197616496 12.4230 11.5346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33957_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 33957_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:20:59.02 -20:38:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 206979_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 206979_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:30:44.04 -18:54:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.454 4121856577550423424 262.68309853449 -18.90685989273 13.0602 11.2902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53174_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 53174_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:06:19.03 -19:32:38.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136162_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 136162_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:23:47.25 -15:06:54.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82720_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 82720_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:18.87 -18:03:47.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49619_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 49619_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:19:07.85 -19:36:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63374_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 63374_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46826_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 46826_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:12:06.02 -19:56:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 5.696 4094261760578288256 273.02676574302 -19.93899200724 9.6902 8.2573 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42670_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 42670_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:34:52.43 -20:13:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 3.155 4118399476894877312 263.71809867040 -20.21913564122 11.1135 9.7288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82562_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 82562_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179162_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 179162_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:09:28.16 -14:58:10.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142858_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 142858_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70656_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 70656_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:41.38 -18:35:18.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14096_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 14096_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:03:49.26 -22:14:15.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31292_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 31292_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62271_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 62271_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133746_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 133746_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:55:52.43 -15:07:19.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61300_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 61300_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32153_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 32153_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:18:19.76 -20:43:33.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128344_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 128344_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:04.63 -15:57:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56338_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 56338_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:55.55 -19:18:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49659_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 49659_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:24:39.67 -19:39:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104400_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 104400_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99402_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 99402_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129792_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 129792_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:46.73 -15:52:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175775_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 175775_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 17:21:15.23 -14:38:04.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48166_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 48166_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:50.38 -19:50:31.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194554_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 194554_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:06.59 -19:06:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 2.120 4095484932920624512 272.52799989846 -19.10837508798 10.8655 10.4543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14506_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 14506_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178312_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 178312_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:10:51.86 -14:53:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148434_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
The candidate 148434_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324 did not pass the final checks
**** FOUND 18:11:47.62 -15:48:16.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106388_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
Preparing report for the candidate 106388_fd_Sgr-01-Q2b1x1_2026-03-29_03-50-34_20.00sec_-14.90C_LIGHT_0324
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 67s
Prepared the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
17:50:32.23 -19:01:10.7
18:11:11.91 -17:05:28.3
17:24:29.05 -16:58:43.3
18:11:06.80 -16:59:49.4
17:41:12.50 -16:39:41.6
18:07:48.58 -16:24:23.2
18:09:17.95 -15:27:52.9
17:57:09.27 -15:34:53.7
18:00:22.36 -22:12:21.7
18:03:41.54 -22:10:57.8
18:03:39.34 -22:07:17.6
18:10:26.62 -15:00:16.2
17:45:55.07 -16:39:04.0
18:10:38.31 -16:36:40.7
18:08:25.18 -15:35:35.1
18:10:50.33 -18:33:33.8
18:11:57.31 -18:52:14.9
18:11:47.34 -18:51:42.5
18:11:27.46 -18:27:03.3
17:18:20.73 -18:56:03.5
17:56:45.80 -16:44:23.1
18:05:24.34 -21:23:33.1
18:05:08.88 -20:59:02.6
17:52:02.04 -20:41:57.7
18:10:18.93 -19:28:13.5
18:10:38.70 -19:17:57.4
18:11:36.98 -19:03:05.7
18:10:11.40 -19:02:22.9
18:11:53.28 -18:59:57.2
18:09:48.36 -18:56:56.5
18:12:01.79 -18:47:42.0
18:11:42.79 -18:42:35.5
18:12:00.19 -18:04:25.1
17:33:36.97 -17:17:26.8
########### Completed Sgr-01-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
17:50:32.23 -19:01:10.7
17:45:55.07 -16:39:04.0
18:10:38.31 -16:36:40.7
18:08:25.18 -15:35:35.1
18:10:50.33 -18:33:33.8
18:11:57.31 -18:52:14.9
18:11:47.34 -18:51:42.5
18:11:27.46 -18:27:03.3
17:18:20.73 -18:56:03.5
17:56:45.80 -16:44:23.1
18:07:48.58 -16:24:23.2
17:24:29.05 -16:58:43.3
18:05:24.34 -21:23:33.1
18:03:39.34 -22:07:17.6
18:10:38.70 -19:17:57.4
18:12:01.79 -18:47:42.0
18:11:42.79 -18:42:35.5
17:52:02.04 -20:41:57.7
17:41:12.50 -16:39:41.6
18:09:17.95 -15:27:52.9
18:10:26.62 -15:00:16.2
18:10:18.93 -19:28:13.5
18:10:11.40 -19:02:22.9
18:03:41.54 -22:10:57.8
18:09:48.36 -18:56:56.5
18:12:00.19 -18:04:25.1
17:57:09.27 -15:34:53.7
18:05:08.88 -20:59:02.6
18:11:53.28 -18:59:57.2
18:11:36.98 -19:03:05.7
18:11:11.91 -17:05:28.3
17:33:36.97 -17:17:26.8
18:00:22.36 -22:12:21.7
18:11:06.80 -16:59:49.4
###################################################################################
17:50:32.23 -19:01:10.7 -- asteroid (will NOT add it to exclusion list)
17:45:55.07 -16:39:04.0 -- not an asteroid (will add it to exclusion list)
18:10:38.31 -16:36:40.7 -- not an asteroid (will add it to exclusion list)
18:08:25.18 -15:35:35.1 -- not an asteroid (will add it to exclusion list)
18:10:50.33 -18:33:33.8 -- not an asteroid (will add it to exclusion list)
18:11:57.31 -18:52:14.9 -- not an asteroid (will add it to exclusion list)
18:11:47.34 -18:51:42.5 -- not an asteroid (will add it to exclusion list)
18:11:27.46 -18:27:03.3 -- not an asteroid (will add it to exclusion list)
17:18:20.73 -18:56:03.5 -- asteroid (will NOT add it to exclusion list)
17:56:45.80 -16:44:23.1 -- asteroid (will NOT add it to exclusion list)
18:07:48.58 -16:24:23.2 -- not an asteroid (will add it to exclusion list)
17:24:29.05 -16:58:43.3 -- not an asteroid (will add it to exclusion list)
18:05:24.34 -21:23:33.1 -- not an asteroid (will add it to exclusion list)
18:03:39.34 -22:07:17.6 -- not an asteroid (will add it to exclusion list)
18:10:38.70 -19:17:57.4 -- not an asteroid (will add it to exclusion list)
18:12:01.79 -18:47:42.0 -- not an asteroid (will add it to exclusion list)
18:11:42.79 -18:42:35.5 -- not an asteroid (will add it to exclusion list)
17:52:02.04 -20:41:57.7 -- not an asteroid (will add it to exclusion list)
17:41:12.50 -16:39:41.6 -- not an asteroid (will add it to exclusion list)
18:09:17.95 -15:27:52.9 -- not an asteroid (will add it to exclusion list)
18:10:26.62 -15:00:16.2 -- not an asteroid (will add it to exclusion list)
18:10:18.93 -19:28:13.5 -- not an asteroid (will add it to exclusion list)
18:10:11.40 -19:02:22.9 -- not an asteroid (will add it to exclusion list)
18:03:41.54 -22:10:57.8 -- not an asteroid (will add it to exclusion list)
18:09:48.36 -18:56:56.5 -- not an asteroid (will add it to exclusion list)
18:12:00.19 -18:04:25.1 -- not an asteroid (will add it to exclusion list)
17:57:09.27 -15:34:53.7 -- not an asteroid (will add it to exclusion list)
18:05:08.88 -20:59:02.6 -- not an asteroid (will add it to exclusion list)
18:11:53.28 -18:59:57.2 -- not an asteroid (will add it to exclusion list)
18:11:36.98 -19:03:05.7 -- not an asteroid (will add it to exclusion list)
18:11:11.91 -17:05:28.3 -- not an asteroid (will add it to exclusion list)
17:33:36.97 -17:17:26.8 -- not an asteroid (will add it to exclusion list)
18:00:22.36 -22:12:21.7 -- not an asteroid (will add it to exclusion list)
18:11:06.80 -16:59:49.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
17:24:29.05 -16:58:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:33:36.97 -17:17:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:41:12.50 -16:39:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:45:55.07 -16:39:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:52:02.04 -20:41:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:57:09.27 -15:34:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:00:22.36 -22:12:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:03:39.34 -22:07:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:03:41.54 -22:10:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:05:08.88 -20:59:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:05:24.34 -21:23:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:07:48.58 -16:24:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:08:25.18 -15:35:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:09:17.95 -15:27:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:09:48.36 -18:56:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:11.40 -19:02:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:18.93 -19:28:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:26.62 -15:00:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:38.31 -16:36:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:38.70 -19:17:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:50.33 -18:33:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:06.80 -16:59:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:11.91 -17:05:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:27.46 -18:27:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:36.98 -19:03:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:42.79 -18:42:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:47.34 -18:51:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:53.28 -18:59:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:57.31 -18:52:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:12:00.19 -18:04:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:12:01.79 -18:47:42.0 -- 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)
17:24:29.05 -16:58:43.3 -- a known variable star
17:33:36.97 -17:17:26.8 -- a known variable star
17:41:12.50 -16:39:41.6 -- a known variable star
17:45:55.07 -16:39:04.0 -- a known variable star
17:52:02.04 -20:41:57.7 -- a known variable star
17:57:09.27 -15:34:53.7 -- a known variable star
18:00:22.36 -22:12:21.7 -- a known variable star
18:03:39.34 -22:07:17.6 -- not a known variable star
18:03:41.54 -22:10:57.8 -- a known variable star
18:05:08.88 -20:59:02.6 -- not a known variable star
18:05:24.34 -21:23:33.1 -- a known variable star
18:07:48.58 -16:24:23.2 -- a known variable star
18:08:25.18 -15:35:35.1 -- a known variable star
18:09:17.95 -15:27:52.9 -- not a known variable star
18:09:48.36 -18:56:56.5 -- not a known variable star
18:10:11.40 -19:02:22.9 -- a known variable star
18:10:18.93 -19:28:13.5 -- a known variable star
18:10:26.62 -15:00:16.2 -- a known variable star
18:10:38.31 -16:36:40.7 -- not a known variable star
18:10:38.70 -19:17:57.4 -- not a known variable star
18:10:50.33 -18:33:33.8 -- not a known variable star
18:11:06.80 -16:59:49.4 -- not a known variable star
18:11:11.91 -17:05:28.3 -- not a known variable star
18:11:27.46 -18:27:03.3 -- a known variable star
18:11:36.98 -19:03:05.7 -- not a known variable star
18:11:42.79 -18:42:35.5 -- not a known variable star
18:11:47.34 -18:51:42.5 -- a known variable star
18:11:53.28 -18:59:57.2 -- not a known variable star
18:11:57.31 -18:52:14.9 -- a known variable star
18:12:00.19 -18:04:25.1 -- not a known variable star
18:12:01.79 -18:47:42.0 -- not a known variable star
Found 14 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
31 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
17:24:29.05 -16:58:43.3
17:33:36.97 -17:17:26.8
17:41:12.50 -16:39:41.6
17:45:55.07 -16:39:04.0
17:52:02.04 -20:41:57.7
17:57:09.27 -15:34:53.7
18:00:22.36 -22:12:21.7
18:03:39.34 -22:07:17.6
18:03:41.54 -22:10:57.8
18:05:08.88 -20:59:02.6
18:05:24.34 -21:23:33.1
18:07:48.58 -16:24:23.2
18:08:25.18 -15:35:35.1
18:09:17.95 -15:27:52.9
18:09:48.36 -18:56:56.5
18:10:11.40 -19:02:22.9
18:10:18.93 -19:28:13.5
18:10:26.62 -15:00:16.2
18:10:38.31 -16:36:40.7
18:10:38.70 -19:17:57.4
18:10:50.33 -18:33:33.8
18:11:06.80 -16:59:49.4
18:11:11.91 -17:05:28.3
18:11:27.46 -18:27:03.3
18:11:36.98 -19:03:05.7
18:11:42.79 -18:42:35.5
18:11:47.34 -18:51:42.5
18:11:53.28 -18:59:57.2
18:11:57.31 -18:52:14.9
18:12:00.19 -18:04:25.1
18:12:01.79 -18:47:42.0
17:44:05.59 -15:12:00.8
18:05:18.11 -22:11:30.9
17:28:44.15 -20:57:39.4
18:08:46.09 -16:26:01.7
18:11:02.05 -19:19:44.2
18:09:31.49 -19:17:24.2
18:09:12.28 -14:59:49.3
18:11:38.57 -19:20:51.2
18:10:06.59 -19:06:31.2
17:19:42.29 -14:55:11.5
17:30:44.04 -18:54:24.2
17:41:17.55 -16:55:17.5
17:50:09.11 -15:51:11.1
18:11:59.98 -18:07:17.8
17:24:05.39 -15:08:45.1
18:00:04.95 -15:56:46.9
18:10:37.24 -16:32:03.6
18:10:37.15 -18:27:13.7
17:49:43.66 -15:52:05.6
17:58:34.06 -18:18:43.7
18:09:16.16 -15:27:47.4
18:12:03.48 -19:20:22.9
18:10:10.29 -19:23:45.6
17:43:15.86 -18:46:50.3
18:11:05.84 -16:36:14.6
17:59:48.07 -20:13:19.9
18:01:12.78 -15:19:54.9
18:10:19.34 -16:38:29.8
18:07:12.80 -15:56:26.0
18:04:31.14 -21:36:32.0
18:04:56.14 -21:31:28.7
18:10:55.59 -15:42:27.9
18:11:09.64 -17:05:22.0
17:19:13.02 -20:42:16.2
17:18:11.68 -19:50:59.2
18:07:46.97 -18:52:20.2
17:38:12.55 -16:06:48.1
17:20:34.60 -20:44:11.7
18:07:15.00 -19:31:52.7
18:11:29.49 -19:19:39.1
18:11:50.48 -19:43:15.6
18:11:13.51 -19:54:56.3
18:10:46.68 -19:33:41.5
18:11:07.58 -19:54:46.9
18:11:25.19 -19:02:14.7
18:11:33.11 -19:30:30.3
18:12:02.00 -19:25:17.6
18:11:27.01 -19:54:35.6
18:06:21.40 -19:58:17.9
18:12:12.98 -19:35:23.8
18:11:45.51 -19:36:43.2
18:11:56.91 -19:00:18.8
18:12:05.01 -19:41:43.8
18:04:48.47 -22:02:59.3
18:11:29.65 -18:48:08.5
18:12:01.39 -19:52:54.7
18:11:43.24 -19:45:03.3
18:11:26.43 -19:39:19.2
18:11:25.45 -19:36:19.0
18:11:35.46 -19:49:34.5
18:11:24.22 -19:04:26.3
18:12:01.20 -19:05:07.3
18:11:15.18 -19:04:58.0
18:11:52.80 -19:38:19.5
18:12:09.43 -19:51:35.7
18:11:37.28 -19:24:36.6
18:12:02.38 -19:10:58.5
18:11:36.66 -19:29:34.0
18:11:48.12 -19:21:37.0
18:10:48.95 -19:47:46.9
18:12:10.08 -19:05:23.4
18:11:56.65 -19:07:33.3
18:10:44.21 -19:46:30.7
18:11:56.80 -19:32:58.7
18:10:54.56 -19:32:21.0
18:11:20.04 -19:15:26.5
18:12:03.55 -19:13:28.5
18:10:57.31 -19:53:48.2
18:11:25.48 -18:54:12.3
18:11:34.92 -19:51:31.4
18:11:14.65 -19:55:54.8
18:11:59.38 -19:56:21.5
18:10:57.09 -19:11:53.9
18:11:59.28 -19:36:55.3
18:11:54.75 -19:49:18.3
17:59:25.84 -15:09:13.9
18:12:00.43 -19:35:51.5
18:11:43.32 -14:29:32.1
18:11:41.31 -19:17:29.9
18:11:32.35 -19:52:27.4
17:35:38.50 -14:39:26.0
18:11:25.28 -18:50:47.3
18:10:48.53 -19:44:00.8
18:11:31.56 -18:57:57.5
18:10:55.88 -19:13:42.6
17:35:51.64 -15:50:49.0
18:12:09.27 -19:00:29.3
18:11:34.82 -19:54:33.7
18:11:47.02 -19:31:31.2
18:12:10.84 -19:33:34.4
17:43:19.93 -14:59:07.0
18:11:03.81 -19:39:22.2
17:38:01.00 -15:21:44.1
18:10:50.49 -19:26:04.0
18:11:54.70 -19:34:46.0
17:21:38.35 -14:37:31.9
17:35:14.51 -14:20:40.0
18:12:05.79 -19:55:10.6
17:29:28.93 -17:46:22.0
17:44:22.87 -17:08:46.5
17:54:56.00 -15:21:10.0
17:34:52.43 -20:13:11.8
18:12:06.02 -19:56:20.2
18:11:41.38 -18:35:18.8
18:11:44.96 -18:26:26.1
17:18:28.86 -17:33:20.7
18:06:19.03 -19:32:38.1
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461128.86805459 -observatory 500
22:52:19.16 -08:07:17.7 Mercury (0.5mag)
01:44:56.13 +10:15:31.8 Venus (-3.9mag)
23:27:26.66 -04:39:26.4 Mars (1.2mag)
07:06:22.93 +22:55:51.8 Jupiter (-2.2mag)
00:21:11.10 -00:01:30.9 Saturn (0.9mag)
03:44:17.70 +19:36:24.3 Uranus (5.8mag)
00:08:27.21 -00:30:32.7 Neptune (7.8mag)
20:32:41.83 -22:52:53.7 Pluto (14.5mag)
09:45:51.48 +14:52:40.3 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Mar 29 03:52 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461128.86805459:
07:06:22.48 +22:55:55.3 Io (5.7mag)
07:06:28.80 +22:55:43.0 Europa (5.8mag)
07:06:06.87 +22:56:27.5 Ganymede (5.2mag)
07:06:57.27 +22:54:50.9 Callisto (6.5mag)
07:10:18.29 +22:52:39.2 Himalia (15.2mag)
07:06:27.10 +22:55:43.1 Thebe (16.1mag)
07:10:04.45 +23:19:13.3 Elara (17.2mag)
07:04:04.08 +23:45:07.1 Pasiphae (17.3mag)
07:15:02.97 +22:51:43.2 Carme (18.4mag)
00:21:18.35 -00:01:14.9 Titan (8.8mag)
00:21:11.68 -00:01:28.0 Rhea (10.1mag)
00:21:28.78 +00:00:38.2 Iapetus (11.5mag)
00:21:05.34 -00:01:05.1 Hyperion (14.8mag)
00:23:00.47 +00:09:02.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 29 03:52 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461128.86805459:
13:54:49.30 -00:15:16.1 JWST
17:01:20.05 +44:20:20.9 Chandra
08:47:41.46 -44:55:02.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 29 03:52 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461128.86805459 -observatory 500
18:41:59.55 -27:50:43.5 14.0mag P/2010 H2 (Vales)
04:55:25.88 -70:33:53.4 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:28.41 +31:20:06.5 17.1mag C/2017 K2 (PANSTARRS)
17:30:38.83 +08:25:06.5 17.6mag C/2021 G2 (ATLAS)
23:04:41.81 +28:37:50.6 17.0mag C/2022 E2 (ATLAS)
04:09:21.24 +25:32:15.7 15.8mag C/2022 N2 (PANSTARRS)
09:01:28.60 +31:43:50.5 16.1mag C/2022 QE78 (ATLAS)
08:29:46.48 -02:09:03.2 17.2mag C/2022 R6 (PANSTARRS)
18:56:21.34 +17:00:54.8 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:11.47 -11:45:31.6 17.6mag P/2023 B1 (PANSTARRS)
09:18:00.55 -14:51:16.2 17.5mag C/2023 F3 (ATLAS)
21:33:34.30 +62:00:41.2 17.4mag C/2023 H5 (Lemmon)
19:30:24.01 -03:33:13.0 14.4mag C/2023 R1 (PANSTARRS)
21:41:49.13 +83:41:38.5 17.8mag C/2023 X2 (Lemmon)
06:13:51.73 +63:40:25.3 16.9mag C/2024 A1 (ATLAS)
04:31:05.27 +10:38:31.2 9.8mag C/2024 E1 (Wierzchos)
16:28:57.69 +03:30:01.1 17.4mag C/2024 G6 (ATLAS)
20:14:13.31 +10:44:02.0 14.8mag C/2024 J3 (ATLAS)
03:11:15.71 -25:12:51.5 16.4mag C/2024 T5 (ATLAS)
05:02:55.42 +50:02:43.0 17.6mag C/2025 J1 (Borisov)
14:48:07.67 +28:29:15.0 14.5mag C/2025 L1 (ATLAS)
02:59:23.55 -23:40:14.6 17.7mag C/2025 Q3 (ATLAS)
22:40:02.86 +19:33:39.4 11.3mag C/2025 R3 (PANSTARRS)
13:01:43.60 +01:52:21.0 17.6mag C/2025 Y1 (ATLAS)
01:43:18.39 -00:46:56.7 11.5mag C/2026 A1 (MAPS)
23:06:24.06 +33:22:36.1 14.0mag C/2026 B2 (Sun-Gao)
18:08:27.75 -10:33:24.3 12.8mag 10P/Tempel
15:21:01.39 +04:40:01.4 12.5mag 24P/Schaumasse
11:08:36.74 -02:09:27.4 15.7mag 29P/Schwassmann-Wachmann
17:51:20.97 -10:18:49.4 17.5mag 40P/Vaisala
10:41:19.05 -05:42:38.4 16.6mag 43P/Wolf-Harrington
01:21:36.57 +14:25:08.8 17.1mag 47P/Ashbrook-Jackson
06:40:39.48 +40:40:38.5 17.1mag 63P/Wild
23:05:47.08 -13:39:02.7 15.7mag 65P/Gunn
03:18:16.74 +14:43:24.4 15.9mag 76P/West-Kohoutek-Ikemura
00:27:14.53 +04:43:15.3 14.5mag 78P/Gehrels
22:07:05.38 -14:29:47.3 14.5mag 88P/Howell
01:22:17.79 +15:41:50.2 15.2mag 93P/Lovas
04:23:41.41 +31:14:12.5 16.4mag 123P/West-Hartley
08:11:43.01 +46:29:11.5 16.2mag 124P/Mrkos
02:06:32.20 +12:20:42.5 16.4mag 128P/Shoemaker-Holt
02:13:19.49 +12:12:16.2 17.4mag 131P/Mueller
23:58:04.15 +06:28:50.7 12.0mag 141P/Machholz
00:08:20.17 -01:37:30.4 12.1mag 141P-A/Machholz
23:03:42.97 -04:45:02.3 15.0mag 141P-D/Machholz
00:13:31.73 -10:13:12.5 15.3mag 162P/SidingSpring
10:34:16.39 +31:52:20.7 17.7mag 164P/Christensen
06:04:19.90 +24:39:52.8 17.7mag 198P/ODAS
15:21:30.50 -02:13:29.1 17.1mag 210P/Christensen
20:42:32.72 -15:40:44.4 17.3mag 218P/LINEAR
17:07:09.68 -15:53:57.0 16.2mag 235P/LINEAR
04:57:43.20 +33:01:47.2 16.5mag 240P/NEAT
07:31:39.66 -07:15:46.4 17.6mag 242P/Spahr
15:47:40.09 +05:43:50.1 17.6mag 391P/Kowalski
07:29:06.31 +21:13:50.4 17.6mag 450P/LONEOS
05:11:25.86 +46:05:10.6 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Mar 29 03:52 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:35.79 -79:28:57.30 ASASSN-26bb 2026-02-24.37 16.2
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
-rw-r--r-- 1 apache apache 5.8K Mar 29 03:52 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 29 03:52 tocp_transients_list.txt