This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 27.4117 2461126.9117 9.69 18:20:37.92 -16:10:22.0
15.07714 -0.71383 galactic Sgr Second-epoch detections are separated by 0.9" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4097815171698857856 | 18:20:35.39 -16:10:48.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B0 1958IzKry..20..208P BD-16 4818
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 4097815171698857856,2461126.9117,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4097815171698857856 20260327.4117 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:20:37.92 -16:10:22.0 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4117 2461126.9117 10.32 18:20:43.49 -16:10:28.5
15.08605 -0.73434 galactic Sgr Second-epoch detections are separated by 3.6" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:20:43.49 -16:10:28.5 (user input) | T | P | (position from user input) SpType: em 1922AnHar..97.....C HD 168520
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9117,10.32,0.05,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
target 20260327.4117 10.32CV 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:20:43.49 -16:10:28.5 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_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 4096379003360285312,2461126.9117,11.22,0.05,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 4096379003360285312 20260327.4117 11.22CV 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:18:27.69 -18:24:32.1 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_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 4099488426571976704,2461126.9117,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4099488426571976704 20260327.4117 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:38:31.09 -17:31:40.6 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_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 J185624.55-212104.9,2461126.9117,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185624.55-212104.9 20260327.4117 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:56:23.84 -21:21:09.0 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_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
V0645 Sct,2461126.9117,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0645 Sct 20260327.4117 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:40:15.19 -15:13:49.8 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_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 4085662617576302208,2461126.9117,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4085662617576302208 20260327.4117 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:59:56.39 -19:34:51.7 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_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,2461126.9117,12.66,0.05,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
VARIABLE_NAME 20260327.4117 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:58:59.59 -19:10:37.4 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20_00sec_-14_90C_LIGHT_0444_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: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
First image: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Last image: 2461126.91195203 27.03.2026 09:53:02.655 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.46
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15321
Objects passed selection criteria: 15297
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 13664.2
Average stars matched: 13030 (95.3583 %)
Memory usage VmPeak: 121608 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 Fri Mar 27 06:43:59 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: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
First image: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Last image: 2461126.91195203 27.03.2026 09:53:02.655 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 64
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.06
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: 58 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): 169829
Objects passed selection criteria: 169521
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 139995
Average stars matched: 131427 (93.8799 %)
Memory usage VmPeak: 1940552 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 Fri Mar 27 06:48:26 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat to cache
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.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: 2461126.91142282
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits exists and is non-empty
Saving wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits to local_wcs_cache/
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> 'local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits exists and is non-empty
Saving wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits to local_wcs_cache/
'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> 'local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits exists and is non-empty
Saving wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits to local_wcs_cache/
'wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits' -> 'local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits'
wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits exists and is non-empty
Saving wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits to local_wcs_cache/
'wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits' -> 'local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:07.809 -18:01:49.83
Angular distance between the image centers 0.05 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 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:06.924 -18:02:11.41
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:40:07.809 -18:01:49.83
Second-epoch second image center 18:40:06.924 -18:02:11.41
Angular distance between the image centers 0.00694 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits &> /tmp/tmp.vvt7YuQiDL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits &> /tmp/tmp.vzPo4HlQjL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits &> /tmp/tmp.8WA46tDvu0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits &> /tmp/tmp.ET4jgJqhrs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
The reference image (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits) and catalog (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat) found
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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 12239 out of 18356 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.804368
a=0.000000 b=1.000000 c=22.804368
From vast_summary.log: estimated ref. image limiting mag.: -8.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
2.1 pix Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
3.1 pix fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
3.1 pix fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
Limiting magnitude estimates:
14.3 mag. Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
14.5 mag. Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
13.8 mag. fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
13.8 mag. fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.2 (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.vvt7YuQiDL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1700, passed=18356
Got 18356 stars (including 16644 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
util/solve_plate_with_UCAC5 got 18356 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 943 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: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 939 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits -region wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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.vzPo4HlQjL (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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1941, passed=20338
Got 20338 stars (including 18376 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
util/solve_plate_with_UCAC5 got 20338 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 942 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 938 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits -region wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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.8WA46tDvu0 (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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=591, passed=11446
Got 11446 stars (including 10842 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat
util/solve_plate_with_UCAC5 got 11446 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 928 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: 0.83"
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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.83"
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 921 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.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.ET4jgJqhrs (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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=619, passed=11841
Got 11841 stars (including 11218 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat
util/solve_plate_with_UCAC5 got 11841 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 931 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: 0.84"
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 931 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: 0.95"
Excluding outliers - 924 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
Saving fully-calibrated image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits'
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits'
Preparing the HTML report for the field Sgr-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out22502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22515.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22502_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
Preparing report for the candidate 22502_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22506_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
Preparing report for the candidate 22506_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22515_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
Preparing report for the candidate 22515_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03666_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 03666_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:57:43.56 -21:06:20.2 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 18s
Prepared the HTML report for the field Sgr-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:20:37.92 -16:10:22.0
18:20:43.49 -16:10:28.5
18:18:27.69 -18:24:32.1
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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat to cache
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Creating symlink local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits exists and is non-empty
wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits exists and is non-empty
wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits exists and is non-empty
wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:07.809 -18:01:49.83
Angular distance between the image centers 0.05 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 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:06.924 -18:02:11.41
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:40:07.809 -18:01:49.83
Second-epoch second image center 18:40:06.924 -18:02:11.41
Angular distance between the image centers 0.00694 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits &> /tmp/tmp.v4aqkwvS7i
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits &> /tmp/tmp.nNHVmiXYG9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits &> /tmp/tmp.6QlA1A4iEH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits &> /tmp/tmp.Tr4wxdnvE3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
The reference image (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits) and catalog (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat) found
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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 16072 out of 204414 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.510618
a=0.000000 b=1.000000 c=22.510618
From vast_summary.log: estimated ref. image limiting mag.: -8.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 47 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
2.1 pix Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
3.2 pix fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
3.1 pix fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
Limiting magnitude estimates:
14.5 mag. Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
14.6 mag. Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
13.7 mag. fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
13.8 mag. fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.v4aqkwvS7i (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=26568, passed=204377
Got 204377 stars (including 177585 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
util/solve_plate_with_UCAC5 got 204377 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 942 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: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits -region wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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.nNHVmiXYG9 (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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=30504, passed=224228
Got 224228 stars (including 193440 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
util/solve_plate_with_UCAC5 got 224228 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 944 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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 939 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits -region wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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.6QlA1A4iEH (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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=8329, passed=90858
Got 90858 stars (including 82450 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat
util/solve_plate_with_UCAC5 got 90858 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.82"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 928 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.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.Tr4wxdnvE3 (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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=9275, passed=97668
Got 97668 stars (including 88313 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat
util/solve_plate_with_UCAC5 got 97668 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 937 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: 0.78"
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 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.78"
Estimated accuracy of the plate solution: 0.87"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Saving fully-calibrated image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-52-16_20.00sec_-14.90C_LIGHT_0444.fits
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.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_2026-03-27_CI_Sgr-02-Q2b1x1_064141_TTUQ2b1x1_28012_JPZeMt32/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445.fits
Preparing the HTML report for the field Sgr-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out110948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out248275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248463.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 4s
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Considering the candidate 248263_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248263_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:42:10.66 -15:36:27.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)
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Considering the candidate 248267_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248267_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:56:02.09 -17:23:22.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 248269_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248269_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:19:39.70 -16:42:21.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 248275_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
Preparing report for the candidate 248275_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
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Considering the candidate 248279_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248279_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:14:25.78 -15:32:39.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 248280_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248280_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:37:21.76 -15:27:54.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)
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Considering the candidate 248284_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248284_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:13:35.25 -14:02:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248286_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248286_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:20:32.91 -13:42:58.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 248289_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248289_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:48:32.99 -21:41:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 4.745 4078974868152934912 282.13860057817 -21.69032975421 12.2694 11.8967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248295_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248295_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:33:55.01 -16:23:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.951 4102813311041655296 278.48050175070 -16.39184313426 12.7127 11.5266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248298_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248298_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:56:30.51 -18:54:59.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
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Considering the candidate 248299_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248299_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:17:48.17 -16:38:50.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)
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Considering the candidate 248302_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248302_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:21:28.62 -15:35:58.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)
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Considering the candidate 248304_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248304_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:31:42.01 -14:29:05.0 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 248307_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
Preparing report for the candidate 248307_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
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Considering the candidate 248323_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248323_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:12:14.29 -15:23:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.846 4145997940229003904 273.06033431284 -15.39931395710 10.1868 8.6039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248324_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248324_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:12:12.24 -20:54:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 4.917 4093988806851276544 273.05117232300 -20.91182859219 11.7243 10.4661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248325_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248325_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:48:20.88 -19:12:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248326_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248326_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:36:48.14 -17:13:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248328_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248328_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 248329_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
Preparing report for the candidate 248329_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
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Considering the candidate 248359_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
Preparing report for the candidate 248359_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
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Considering the candidate 248360_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248360_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:15:26.95 -18:40:34.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248377_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248377_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:42:58.92 -19:14:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248385_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248385_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:13:45.64 -21:01:38.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 248412_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248412_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:31:32.32 -14:16:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248415_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248415_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:54:36.06 -15:36:06.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248429_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248429_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:19:46.63 -17:44:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248434_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248434_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:36:44.63 -17:13:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248438_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248438_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 248439_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248439_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:29:40.22 -16:39:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.134 4096856260115170816 277.41769437771 -16.65972679902 12.0119 10.8615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248454_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 248454_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:35:27.50 -20:50:39.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248463_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
Preparing report for the candidate 248463_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
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Considering the candidate 110948_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 110948_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:55:57.00 -17:39:54.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)
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Considering the candidate 217502_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 217502_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:50:57.38 -21:50:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78421_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 78421_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:42:55.03 -19:17:03.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 70894_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 70894_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:46:01.03 -19:36:21.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 95215_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 95215_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:31:26.35 -18:24:08.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 39718_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 39718_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:38:53.26 -21:03:08.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53867_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 53867_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:49:39.96 -20:19:26.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141366_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 141366_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:55:30.84 -16:22:40.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193095_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 193095_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:54:42.96 -15:36:10.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 34778_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 34778_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:53:59.97 -21:21:34.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 48151_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 48151_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:25:21.19 -20:32:27.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 47520_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 47520_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:57:20.28 -20:39:20.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 40525_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 40525_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks
**** FOUND 18:57:43.53 -21:06:20.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 35696_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445
The candidate 35696_fd_Sgr-02-Q2b1x1_2026-03-27_04-53-02_20.00sec_-15.00C_LIGHT_0445 did not pass the final checks