This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1806897487383595136,2461126.9139,12.88,0.05,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 1806897487383595136 20260327.4139 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:06:58.30 +14:40:25.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_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 1808094099632949120,2461126.9139,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1808094099632949120 20260327.4139 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:04:49.09 +16:06:54.0 ;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_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4139 2461126.9139 12.71 20:02:59.65 +15:18:35.0
54.89099 -8.23792 galactic Aql Second-epoch detections are separated by 4.6" and 1.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.7441+15.3057 | 20:02:58.61 +15:18:33.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.7441+15.3057,2461126.9139,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.7441+15.3057 20260327.4139 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:02:59.65 +15:18:35.0 ;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_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J201258+1425.5,2461126.9139,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J201258+1425.5 20260327.4139 11.98CV 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/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:58.63 +14:25:35.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4139 2461126.9139 12.45 20:29:01.65 +16:17:06.3
59.14347 -13.00323 galactic Del Second-epoch detections are separated by 4.4" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J307.2654+16.2897 | 20:29:01.65 +16:17:06.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4139* 20 29 01.65 +16 17 06.3 12.4 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J307.2654+16.2897,2461126.9139,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J307.2654+16.2897 20260327.4139 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:29:01.65 +16:17:06.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4139* 20 46 39.96 +16 05 07.7 12.7 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1762999172103487616,2461126.9139,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1762999172103487616 20260327.4139 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:46:39.96 +16:05:07.7 ;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_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4139* 20 37 49.37 +13 58 02.6 13.0 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J203749.65+135748.5,2461126.9139,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J203749.65+135748.5 20260327.4139 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:37:49.37 +13:58:02.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4139 2461126.9139 13.13 20:30:05.19 +17:33:40.7
60.37451 -12.50194 galactic Del Second-epoch detections are separated by 2.7" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J307.5244+17.5569 | 20:30:05.19 +17:33:40.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4139* 20 30 05.19 +17 33 40.7 13.1 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J307.5244+17.5569,2461126.9139,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J307.5244+17.5569 20260327.4139 13.13CV 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/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:30:05.19 +17:33:40.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4139* 20 25 02.05 +11 12 37.6 11.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CK Del,2461126.9139,11.52,0.05,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
CK Del 20260327.4139 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:02.05 +11:12:37.6 ;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_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_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 1806674630114821248,2461126.9139,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1806674630114821248 20260327.4139 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:02.55 +14:12:59.6 ;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_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4139 2461126.9139 12.72 20:20:54.86 +14:16:04.5
56.31539 -12.46695 galactic Del Second-epoch detections are separated by 0.8" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.2290+14.2665 | 20:20:54.86 +14:16:04.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4139* 20 20 54.86 +14 16 04.5 12.7 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J305.2290+14.2665,2461126.9139,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J305.2290+14.2665 20260327.4139 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:20:54.86 +14:16:04.5 ;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_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png resample_wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20_00sec_-15_00C_LIGHT_0448_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: 2461094.00795693 22.02.2026 12:11:17.479 /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
First image: 2461094.00795693 22.02.2026 12:11:17.479 /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
Last image: 2461126.91415626 27.03.2026 09:56:13.101 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.25
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): 15751
Objects passed selection criteria: 15735
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: 14068.8
Average stars matched: 13672 (97.1799 %)
Memory usage VmPeak: 120900 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 05:43:57 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: 2461094.00795693 22.02.2026 12:11:17.479 /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
First image: 2461094.00795693 22.02.2026 12:11:17.479 /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
Last image: 2461126.91415626 27.03.2026 09:56:13.101 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 200
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.90
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: 49 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): 121891
Objects passed selection criteria: 121693
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 103264
Average stars matched: 99259.8 (96.1219 %)
Memory usage VmPeak: 1951440 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 05:46:13 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/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
SExtractor catalog cache: saved Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat to cache
SExtractor catalog cache: saved Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.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/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.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: 2461126.91364066
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits exists and is non-empty
Saving wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits to local_wcs_cache/
'wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits' -> 'local_wcs_cache/wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits'
wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits exists and is non-empty
Saving wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits to local_wcs_cache/
'wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits' -> 'local_wcs_cache/wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits'
wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits exists and is non-empty
Saving wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits to local_wcs_cache/
'wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits' -> 'local_wcs_cache/wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits'
wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits exists and is non-empty
Saving wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits to local_wcs_cache/
'wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits' -> 'local_wcs_cache/wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits'
The image scale is 5.89"/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 20:26:47.833 +14:00:00.87
Second-epoch image center 20:26:43.699 +13:55:48.65
Angular distance between the image centers 0.07 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 20:26:47.833 +14:00:00.87
Second-epoch image center 20:26:44.427 +13:55:46.88
Angular distance between the image centers 0.07 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 20:26:43.699 +13:55:48.65
Second-epoch second image center 20:26:44.427 +13:55:46.88
Angular distance between the image centers 0.00298 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/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits &> /tmp/tmp.LzC8Gg8Rs4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits &> /tmp/tmp.vYVDn1KyTl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits &> /tmp/tmp.c4XmpsiNhI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits &> /tmp/tmp.4kTI2mHj41
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
Calibrating the magnitude scale
Found non-empty wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.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_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits and wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.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_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits and wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat
Found non-empty wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits and wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat
The reference image (wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits) and catalog (wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat) found
'wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.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 12257 out of 17752 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.720509
a=0.000000 b=1.000000 c=22.720509
From vast_summary.log: estimated ref. image limiting mag.: -8.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
2.5 pix Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
3.1 pix fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
3.3 pix fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
Limiting magnitude estimates:
14.5 mag. Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
14.5 mag. Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
14.0 mag. fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
13.9 mag. fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.4 (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.LzC8Gg8Rs4 (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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits' -> 'wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
WCS_IMAGE_NAME=wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
WCS-calibrated image found: wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
Checking if the catalog wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat corresponding to the image wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits alredy exist and is non-empty...
Catalog wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat corresponding to the image wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
WCS catalog name: wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat
SExtractor catalog parsing summary: zero_flux=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1482, passed=17746
Got 17746 stars (including 16246 good ones) from the SExtractor catalog wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat
util/solve_plate_with_UCAC5 got 17746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 939 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: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits -region wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.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.vYVDn1KyTl (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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits' -> 'wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
WCS_IMAGE_NAME=wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
WCS-calibrated image found: wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
Checking if the catalog wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat corresponding to the image wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits alredy exist and is non-empty...
Catalog wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat corresponding to the image wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
WCS catalog name: wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1460, passed=17504
Got 17504 stars (including 16027 good ones) from the SExtractor catalog wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat
util/solve_plate_with_UCAC5 got 17504 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 940 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: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 935 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits -region wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.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.c4XmpsiNhI (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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
WCS_IMAGE_NAME=wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
WCS-calibrated image found: wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
Checking if the catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat corresponding to the image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits alredy exist and is non-empty...
Catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat corresponding to the image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
WCS catalog name: wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=637, passed=13479
Got 13479 stars (including 12837 good ones) from the SExtractor catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat
util/solve_plate_with_UCAC5 got 13479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.74"
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: 0.74"
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits -region wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.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.4kTI2mHj41 (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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
WCS_IMAGE_NAME=wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
WCS-calibrated image found: wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
Checking if the catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat corresponding to the image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits alredy exist and is non-empty...
Catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat corresponding to the image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
WCS catalog name: wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=599, passed=12566
Got 12566 stars (including 11962 good ones) from the SExtractor catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat
util/solve_plate_with_UCAC5 got 12566 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 932 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 932 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: 0.79"
Excluding outliers - 923 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits -region wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.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_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits'
Saving fully-calibrated image wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits'
Saving fully-calibrated image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits'
Saving fully-calibrated image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits'
Preparing the HTML report for the field Del-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21103.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20978_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 20978_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:49:53.16 +12:03:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.98, MAG_FAINT_SEARCH_LIMIT=11.96)GAIADR2_OUTPUT=# 0.175 1757903176218768384 312.47145961867 +12.05091723931 10.6460 10.3242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21008_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 21008_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:11.97 +12:05:01.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21103_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 21103_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:51:10.46 +12:21:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.09, MAG_FAINT_SEARCH_LIMIT=11.07)GAIADR2_OUTPUT=# 0.228 1757938536686477056 312.79351884895 +12.36579830730 9.6381 9.2035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21215_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 21215_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:31:07.27 +11:31:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21413_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 21413_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 19:58:46.37 +16:12:47.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21481_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 21481_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:42:24.72 +15:20:14.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21521_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 21521_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:06:09.93 +12:13:03.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05989_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 05989_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:12:44.89 +12:59:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10208_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 10208_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:11:37.55 +15:37:14.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Del-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
SExtractor catalog cache: saved Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat to cache
SExtractor catalog cache: saved Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
Creating symlink local_wcs_cache/wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
Creating symlink local_wcs_cache/wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
Creating symlink local_wcs_cache/wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.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_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits exists and is non-empty
wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits exists and is non-empty
wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits exists and is non-empty
wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits exists and is non-empty
The image scale is 5.89"/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 20:26:47.833 +14:00:00.87
Second-epoch image center 20:26:43.699 +13:55:48.65
Angular distance between the image centers 0.07 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 20:26:47.833 +14:00:00.87
Second-epoch image center 20:26:44.427 +13:55:46.88
Angular distance between the image centers 0.07 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 20:26:43.699 +13:55:48.65
Second-epoch second image center 20:26:44.427 +13:55:46.88
Angular distance between the image centers 0.00298 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/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits &> /tmp/tmp.1aVkwKs7jm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits &> /tmp/tmp.DsHoknlJP4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits &> /tmp/tmp.7iTvG1NMfU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits &> /tmp/tmp.4knIAwr16m
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
Calibrating the magnitude scale
Found non-empty wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.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_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits and wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.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_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits and wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat
Found non-empty wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits and wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat
The reference image (wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits) and catalog (wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat) found
'wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.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 15276 out of 136475 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.453863
a=0.000000 b=1.000000 c=22.453863
From vast_summary.log: estimated ref. image limiting mag.: -7.90
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.55
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.55
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 122 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
2.4 pix Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
3.1 pix fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
3.3 pix fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
Limiting magnitude estimates:
14.6 mag. Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
14.5 mag. Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
14.0 mag. fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
13.9 mag. fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.2 (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.1aVkwKs7jm (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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits' -> 'wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
WCS_IMAGE_NAME=wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
WCS-calibrated image found: wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
Checking if the catalog wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat corresponding to the image wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits alredy exist and is non-empty...
Catalog wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat corresponding to the image wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
WCS catalog name: wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat
SExtractor catalog parsing summary: zero_flux=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=17544, passed=136446
Got 136446 stars (including 118722 good ones) from the SExtractor catalog wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat
util/solve_plate_with_UCAC5 got 136446 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 939 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 936 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits -region wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.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.DsHoknlJP4 (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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits' -> 'wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
WCS_IMAGE_NAME=wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
WCS-calibrated image found: wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
Checking if the catalog wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat corresponding to the image wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits alredy exist and is non-empty...
Catalog wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat corresponding to the image wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
WCS catalog name: wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat
SExtractor catalog parsing summary: zero_flux=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=17274, passed=135315
Got 135315 stars (including 117876 good ones) from the SExtractor catalog wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat
util/solve_plate_with_UCAC5 got 135315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 940 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: 0.63"
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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 934 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_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits -region wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.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.7iTvG1NMfU (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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
WCS_IMAGE_NAME=wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
WCS-calibrated image found: wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
Checking if the catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat corresponding to the image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits alredy exist and is non-empty...
Catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat corresponding to the image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
WCS catalog name: wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=7381, passed=86585
Got 86585 stars (including 79109 good ones) from the SExtractor catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat
util/solve_plate_with_UCAC5 got 86585 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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 934 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: 0.74"
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 934 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: 0.77"
Excluding outliers - 924 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits -region wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.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.4knIAwr16m (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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
WCS_IMAGE_NAME=wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
WCS-calibrated image found: wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
Checking if the catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat corresponding to the image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits alredy exist and is non-empty...
Catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat corresponding to the image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
WCS catalog name: wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=7123, passed=77793
Got 77793 stars (including 70604 good ones) from the SExtractor catalog wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat
util/solve_plate_with_UCAC5 got 77793 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 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: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 925 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits -region wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.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_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/wcs_Del-01-Q2b1x1_2026-02-22_06-11-17_20.00sec_-15.00C_LIGHT_0496.fits
Saving fully-calibrated image wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/wcs_Del-01-Q2b1x1_2026-02-22_06-12-06_20.00sec_-15.00C_LIGHT_0497.fits
Saving fully-calibrated image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/wcs_fd_Del-01-Q2b1x1_2026-03-27_04-55-28_20.00sec_-15.00C_LIGHT_0448.fits
Saving fully-calibrated image wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.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_Del-01-Q2b1x1_054141_TTUQ2b1x1_24554_QvXd6vhY/wcs_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449.fits
Preparing the HTML report for the field Del-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out122234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160182.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out158403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61008.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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: 7s
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Considering the candidate 158359_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158359_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:46:04.19 +14:59:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.118 1762313248637558016 311.51598705272 +14.99475378464 13.4896 12.9672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158365_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158365_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:23:38.93 +16:06:48.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 158366_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158366_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:45:30.43 +17:32:40.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 158375_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158375_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 158378_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158378_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:47:38.40 +17:17:38.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 158379_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158379_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:09:58.74 +14:43:37.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)
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Considering the candidate 158383_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158383_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:21:35.14 +10:07:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.427 1753501835472094208 305.39546564503 +10.11792498321 12.8242 11.9235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158384_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158384_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:43:27.44 +10:16:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158387_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158387_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:06:45.36 +15:32:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158401_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158401_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:42:49.59 +17:49:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158402_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158402_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:01:31.64 +11:04:42.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)
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Considering the candidate 158403_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 158403_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 158405_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158405_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:07:39.17 +10:28:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158406_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158406_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:37:38.62 +17:55:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158408_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158408_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 19:59:42.06 +12:25:13.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)
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Considering the candidate 158410_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158410_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:28:32.80 +12:07:42.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 158417_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158417_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:48:10.51 +15:35:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 3.180 1762921931402697216 312.04458663842 +15.58908756204 12.7320 12.0407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158419_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 158419_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 158420_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158420_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:03:18.02 +16:13:49.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 158424_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 158424_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 158429_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158429_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:07:55.02 +13:29:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.631 1806153633407334016 301.97864142563 +13.48354338506 12.8985 12.4241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158432_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158432_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:00:09.79 +18:04:23.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)
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Considering the candidate 158438_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158438_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:06:04.01 +17:56:52.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)
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Considering the candidate 158444_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158444_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:12.97 +12:19:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.079 1757940147297243776 312.55348002175 +12.32290233326 12.0371 11.3979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158451_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158451_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:48:39.57 +17:48:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158452_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 158452_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 158453_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158453_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:40:30.38 +16:33:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158455_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158455_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:49:53.19 +12:03:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 0.766 1757903176218768384 312.47145961867 +12.05091723931 10.6460 10.3242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158485_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158485_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:11.97 +12:05:01.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 158578_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158578_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:51:10.46 +12:21:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.11, MAG_FAINT_SEARCH_LIMIT=11.09)GAIADR2_OUTPUT=# 0.320 1757938536686477056 312.79351884895 +12.36579830730 9.6381 9.2035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158682_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158682_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:51:04.87 +12:12:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.70, MAG_FAINT_SEARCH_LIMIT=11.68)GAIADR2_OUTPUT=# 0.794 1757923173587029888 312.77007612551 +12.20832398803 10.2146 9.6601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158948_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 158948_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:51:12.25 +12:11:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159094_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 159094_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 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 159381_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 159381_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 159545_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 159545_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:45.26 +11:59:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.686 1757892425917492608 312.68857476418 +11.99150397879 11.7352 11.1686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159742_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 159742_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:08:10.08 +16:38:02.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 159832_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 159832_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 159932_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 159932_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:20.93 +12:09:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.737 1757911392493199872 312.58719799978 +12.16618445037 11.9119 11.1974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159933_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 159933_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 159986_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 159986_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:45:04.34 +12:41:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.783 1755188898624521728 311.26765880862 +12.68470085657 12.3128 11.8024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160182_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160182_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:26.52 +11:59:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 0.314 1757895174696613376 312.61050479794 +11.99607951721 12.1847 11.7563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160279_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160279_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 160330_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160330_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:30:43.49 +14:43:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 0.749 1804605246144811776 307.68141971371 +14.72837170068 12.7530 12.4874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160348_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160348_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 160361_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160361_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:44:11.38 +15:09:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160373_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 160373_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 160390_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160390_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:13.76 +12:02:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.987 1757908020941878784 312.55695756564 +12.04311584244 12.2962 11.5581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160401_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160401_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:35:21.88 +11:21:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160580_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160580_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:56.67 +13:10:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 4.654 1761128288638015616 312.73491304742 +13.17855499764 12.5282 12.0313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160749_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160749_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 160773_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160773_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 160825_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160825_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:24:25.06 +14:12:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.369 1804971246077378048 306.10475380175 +14.20847224550 12.9348 12.0452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160831_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160831_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:48.52 +11:51:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.670 1757884488817862400 312.70176143046 +11.86239834576 12.4936 11.9952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160836_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160836_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:49:48.99 +11:58:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.358 1757901492591590656 312.45392824759 +11.97542557607 12.5801 12.1416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160911_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160911_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:51:33.74 +13:06:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.140 1761081177139213952 312.89016264033 +13.11315270446 12.4507 11.9405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160916_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160916_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:23:07.11 +09:47:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160952_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160952_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 160960_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160960_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:40:25.06 +13:27:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160974_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160974_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 160979_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160979_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 160990_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 160990_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:27:12.98 +12:55:27.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 161016_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161016_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:28.31 +16:35:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161065_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 161065_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 161156_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 161156_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 161162_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161162_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 161165_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161165_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 161229_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161229_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:44.66 +12:06:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.185 1757898297136453504 312.68636862937 +12.10259983931 12.2919 11.1825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161235_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161235_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:35.74 +11:58:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.693 1757894934178411008 312.64893097566 +11.97685861316 12.6661 12.2063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161260_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161260_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:59.11 +13:25:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 5.400 1761159727798678784 312.74517124391 +13.41627491192 12.8903 12.1573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161301_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161301_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 161310_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161310_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 161323_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161323_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:39:48.71 +10:04:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161365_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161365_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:51:10.51 +12:27:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.423 1757947878243971968 312.79339387664 +12.45021137806 12.8780 12.7168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161376_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161376_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 161379_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161379_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:51:05.45 +12:48:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.799 1761054140322876416 312.77191597175 +12.81205885137 13.0723 12.5823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161394_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161394_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:26:40.33 +12:29:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161560_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161560_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 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 161562_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161562_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:57.33 +13:58:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.200 1761382035306630272 312.73967660902 +13.97168100657 13.0168 12.5124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161586_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161586_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 161602_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161602_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 161617_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161617_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 161627_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161627_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 161644_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161644_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 161668_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161668_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:51:17.18 +12:34:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.532 1757951249789877120 312.82162890526 +12.57041865022 12.9622 12.4594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161756_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161756_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 161769_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161769_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:51:28.50 +16:29:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161784_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161784_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:43:05.69 +09:41:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161794_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161794_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:26:45.61 +13:22:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.427 1804116680725612672 306.68987051906 +13.38012448014 13.6832 13.2255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161837_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161837_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:43:13.60 +10:15:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161841_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161841_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:43:03.58 +11:45:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.499 1754847221087827968 310.76477888395 +11.75049631715 13.4449 12.8595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161850_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161850_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 161860_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161860_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 161879_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161879_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 161881_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161881_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 161884_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161884_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:52:01.87 +15:06:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.996 1761985907706940032 313.00737583504 +15.10383968934 13.5332 12.8612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161905_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161905_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:48:12.37 +12:13:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161931_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161931_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:45:23.09 +12:14:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161932_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161932_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:27:17.06 +14:30:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161935_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161935_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 161947_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161947_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:07.36 +12:09:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161983_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161983_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 161994_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161994_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 161995_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 161995_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:50:41.99 +13:19:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.952 1761135156288240384 312.67442009097 +13.31799903200 13.3840 12.6853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 162018_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 162018_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 162023_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 162023_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 162052_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 162052_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 162062_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 162062_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 162075_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 162075_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:37:07.02 +13:46:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.805 1756296033816929664 309.27873613810 +13.77264741622 13.7327 13.3035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 162103_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 162103_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 40471_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 40471_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:12:44.88 +12:59:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22871_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 22871_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 156377_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 156377_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 84909_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 84909_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:42:24.71 +15:20:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22430_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 22430_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 93069_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 93069_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:42:16.16 +17:20:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57386_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 57386_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 78250_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 78250_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:11:37.57 +15:37:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61008_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
Preparing report for the candidate 61008_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
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Considering the candidate 28005_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 28005_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:31:07.27 +11:31:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122234_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 122234_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:23:34.72 +17:09:09.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)
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Considering the candidate 49383_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 49383_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks
**** FOUND 20:04:32.77 +13:48:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118011_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449
The candidate 118011_fd_Del-01-Q2b1x1_2026-03-27_04-56-13_20.00sec_-14.90C_LIGHT_0449 did not pass the final checks