This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 21.1536 2461120.6536 11.74 09:01:33.53 -35:49:54.0
259.41195 6.95407 galactic Pyx Second-epoch detections are separated by 0.5" and 4.2 pix
The object was found in VSX 1" ASAS J090134-3550.0
Type: M
# Max. Min./Amp. JD0 Period
10.910 V Y 2.120 CV 2452567.80000 354.861604000000 Ce
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J090134-3550.0,2461120.6536,11.74,0.05,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
ASAS J090134-3550.0 20260321.1536 11.74CV 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/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:33.53 -35:49:54.0 ;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_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20_00sec_-15_00C_LIGHT_0116_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20_00sec_-14_90C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20_00sec_-15_00C_LIGHT_0116_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20_00sec_-14_90C_LIGHT_0115_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1536 2461120.6536 10.98 09:40:46.88 -36:43:32.7
265.65301 11.98991 galactic Ant Second-epoch detections are separated by 0.4" and 4.2 pix
The object was found in VSX 3" ASAS J094047-3643.5
Type: MISC
# Max. Min./Amp. JD0 Period
12.170 V Y 1.390 V 2452758.00000 311.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 21.1536* 09 40 46.88 -36 43 32.7 11.0 U Ant 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
ASAS J094047-3643.5,2461120.6536,10.98,0.05,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 J094047-3643.5 20260321.1536 10.98CV 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/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:40:46.88 -36:43:32.7 ;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_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20_00sec_-15_00C_LIGHT_0116_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20_00sec_-14_90C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20_00sec_-15_00C_LIGHT_0116_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20_00sec_-14_90C_LIGHT_0115_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1536 2461120.6536 12.14 09:48:33.16 -35:43:08.1
266.16859 13.78364 galactic Ant Second-epoch detections are separated by 0.5" and 4.2 pix
The object was found in VSX 2" ASAS J094833-3543.1
Type: M
# Max. Min./Amp. JD0 Period
10.980 V Y 1.330 CV 2452193.90000 142.600000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 21.1536* 09 48 33.16 -35 43 08.1 12.1 U Ant 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
ASAS J094833-3543.1,2461120.6536,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J094833-3543.1 20260321.1536 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:48:33.16 -35:43:08.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20_00sec_-15_00C_LIGHT_0116_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20_00sec_-14_90C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20_00sec_-15_00C_LIGHT_0116_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20_00sec_-14_90C_LIGHT_0115_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 21.1536* 09 05 45.03 -37 39 38.4 11.5 U Vel 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
V0480 Vel,2461120.6536,11.52,0.05,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
V0480 Vel 20260321.1536 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/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:45.03 -37:39:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20_00sec_-15_00C_LIGHT_0116_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20_00sec_-14_90C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20_00sec_-15_00C_LIGHT_0116_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20_00sec_-14_90C_LIGHT_0115_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: 2461049.85665904 09.01.2026 08:33:25.341 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
First image: 2461049.85665904 09.01.2026 08:33:25.341 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
Last image: 2461120.65386777 21.03.2026 03:41:24.175 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.45
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): 9636
Objects passed selection criteria: 9633
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 9222.25
Average stars matched: 8910.5 (96.6196 %)
Memory usage VmPeak: 115424 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 22:49:32 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: 2461049.85665904 09.01.2026 08:33:25.341 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
First image: 2461049.85665904 09.01.2026 08:33:25.341 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
Last image: 2461120.65386777 21.03.2026 03:41:24.175 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 146
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.16
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: 47 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): 84725
Objects passed selection criteria: 84582
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 80521
Average stars matched: 77649.2 (96.4335 %)
Memory usage VmPeak: 2175400 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 22:51:39 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/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
SExtractor catalog cache: saved Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.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/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.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: 2461120.65334087
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits exists and is non-empty
Saving wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits to local_wcs_cache/
'wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits'
wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits exists and is non-empty
Saving wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits to local_wcs_cache/
'wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits'
wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits exists and is non-empty
Saving wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits to local_wcs_cache/
'wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits' -> 'local_wcs_cache/wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits'
wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits exists and is non-empty
Saving wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits to local_wcs_cache/
'wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits' -> 'local_wcs_cache/wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:23:28.933 -34:00:00.19
Second-epoch image center 09:23:28.865 -34:00:22.72
Angular distance between the image centers 0.01 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 09:23:28.933 -34:00:00.19
Second-epoch image center 09:23:27.057 -34:00:34.07
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:23:28.865 -34:00:22.72
Second-epoch second image center 09:23:27.057 -34:00:34.07
Angular distance between the image centers 0.00700 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/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits &> /tmp/tmp.h54XTgQcLS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits &> /tmp/tmp.L9tVpHDvD1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits &> /tmp/tmp.yMYBjUwgbM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits &> /tmp/tmp.emdyAxPli9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
Calibrating the magnitude scale
Found non-empty wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.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_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.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_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat
Found non-empty wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat
The reference image (wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits) and catalog (wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat) found
'wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.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 9006 out of 10675 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.742026
a=0.000000 b=1.000000 c=22.742026
From vast_summary.log: estimated ref. image limiting mag.: -8.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.29
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
2.0 pix Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
2.5 pix fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
2.4 pix fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
Limiting magnitude estimates:
14.3 mag. Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
14.3 mag. Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
14.1 mag. fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
14.1 mag. fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.h54XTgQcLS (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits' -> 'wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
Checking if the catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
WCS catalog name: wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=859, passed=10675
Got 10675 stars (including 9809 good ones) from the SExtractor catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 10675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits -region wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.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.L9tVpHDvD1 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits' -> 'wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
Checking if the catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
WCS catalog name: wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=850, passed=10717
Got 10717 stars (including 9854 good ones) from the SExtractor catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 10717 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits -region wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.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.yMYBjUwgbM (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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
WCS-calibrated image found: wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
Checking if the catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
WCS catalog name: wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=653, passed=10731
Got 10731 stars (including 10073 good ones) from the SExtractor catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat
util/solve_plate_with_UCAC5 got 10731 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 961 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: 0.67"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits -region wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.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.emdyAxPli9 (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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
WCS-calibrated image found: wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
Checking if the catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat corresponding to the image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat corresponding to the image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
WCS catalog name: wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=707, passed=10618
Got 10618 stars (including 9906 good ones) from the SExtractor catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat
util/solve_plate_with_UCAC5 got 10618 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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 962 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: 0.68"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits -region wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.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_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits'
Saving fully-calibrated image wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits'
Saving fully-calibrated image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits'
Saving fully-calibrated image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits'
Preparing the HTML report for the field Pyx-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20706.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20632_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20632_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:37:50.06 -36:14:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.30, MAG_FAINT_SEARCH_LIMIT=11.28)GAIADR2_OUTPUT=# 1.772 5436509611173618560 144.45849725496 -36.24306815549 10.3639 9.6941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20653_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20653_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:22:04.50 -36:42:09.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20666_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20666_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:40:46.90 -36:43:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 3.089 5436443335535734272 145.19646384781 -36.72595642911 9.9041 8.4241 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20671_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20671_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:32:12.37 -36:23:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 2.006 5436358123387649664 143.05219077220 -36.39919488323 9.8873 8.4339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20682_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20682_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:21:35.67 -34:19:48.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20687_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20687_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:52:05.97 -33:05:45.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20688_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20688_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:18:23.47 -32:27:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 0.348 5630894883189522944 139.59789129207 -32.46074226421 10.3928 9.2062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20690_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20690_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:37:34.82 -31:02:26.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20691_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20691_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:15:43.91 -34:57:47.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20693_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20693_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:59:52.44 -34:44:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.000 5627358686297146752 134.96867956488 -34.74434810116 10.5008 9.3511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20697_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20697_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:22:25.34 -34:18:17.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20703_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20703_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:24:06.88 -36:05:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20706_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20706_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:13:33.28 -35:31:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 1.341 5623699649037710336 138.38912009876 -35.52664453965 11.1702 10.5904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20707_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 20707_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:28:04.66 -32:44:55.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04861_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 04861_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:33:42.41 -34:43:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09521_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 09521_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:26:34.95 -30:03:20.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Pyx-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
SExtractor catalog cache: saved Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
Creating symlink local_wcs_cache/wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
Creating symlink local_wcs_cache/wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
Creating symlink local_wcs_cache/wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.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_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits exists and is non-empty
wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits exists and is non-empty
wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:23:28.933 -34:00:00.19
Second-epoch image center 09:23:28.865 -34:00:22.72
Angular distance between the image centers 0.01 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 09:23:28.933 -34:00:00.19
Second-epoch image center 09:23:27.057 -34:00:34.07
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:23:28.865 -34:00:22.72
Second-epoch second image center 09:23:27.057 -34:00:34.07
Angular distance between the image centers 0.00700 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/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits &> /tmp/tmp.4rHBPgN3ug
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits &> /tmp/tmp.qKCJo5pz3x
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits &> /tmp/tmp.Q6DZBkGDsV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits &> /tmp/tmp.QCzFeEST2A
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
Calibrating the magnitude scale
Found non-empty wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.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_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.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_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat
Found non-empty wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat
The reference image (wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits) and catalog (wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat) found
'wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.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 14737 out of 94618 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.574739
a=0.000000 b=1.000000 c=22.574739
From vast_summary.log: estimated ref. image limiting mag.: -8.16
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.41
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 92 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
1.9 pix Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
2.3 pix fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
2.3 pix fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
Limiting magnitude estimates:
14.4 mag. Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
14.4 mag. Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
14.3 mag. fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
14.3 mag. fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.4rHBPgN3ug (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits' -> 'wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
Checking if the catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
WCS catalog name: wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=5975, passed=94606
Got 94606 stars (including 88477 good ones) from the SExtractor catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 94606 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits -region wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.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.qKCJo5pz3x (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits' -> 'wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
Checking if the catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat corresponding to the image wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
WCS catalog name: wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=5797, passed=94565
Got 94565 stars (including 88585 good ones) from the SExtractor catalog wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 94565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits -region wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.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.Q6DZBkGDsV (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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
WCS-calibrated image found: wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
Checking if the catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat corresponding to the image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
WCS catalog name: wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=5287, passed=80548
Got 80548 stars (including 75158 good ones) from the SExtractor catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat
util/solve_plate_with_UCAC5 got 80548 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits -region wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.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.QCzFeEST2A (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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
WCS-calibrated image found: wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
Checking if the catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat corresponding to the image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat corresponding to the image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
WCS catalog name: wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=5450, passed=82325
Got 82325 stars (including 76782 good ones) from the SExtractor catalog wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat
util/solve_plate_with_UCAC5 got 82325 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits -region wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.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_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/wcs_Pyx-02-Q2b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits
Saving fully-calibrated image wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/wcs_Pyx-02-Q2b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits
Saving fully-calibrated image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-40-38_20.00sec_-14.90C_LIGHT_0115.fits
Saving fully-calibrated image wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.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_2026-03-20_CI_Pyx-02-Q2b1x1_224209_TTUQ2b1x1_11339_EkAMlU8X/wcs_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116.fits
Preparing the HTML report for the field Pyx-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out104922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112192.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out12889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32836.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112176_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112176_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:26:00.74 -32:45:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.497 5630403440152445568 141.50341665753 -32.75700172120 13.7998 13.2690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112186_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112186_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112188_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112188_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:57:43.56 -30:07:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 3.071 5641515345181865472 134.43155118262 -30.12707425478 13.9461 13.1844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112192_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112192_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:22:05.92 -36:22:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.328 5431283739786959360 140.52524061133 -36.36856360218 13.5808 12.9784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112194_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112194_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:37:11.73 -30:45:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.371 5632403589238083456 144.29931805817 -30.76525762838 13.9935 13.3237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112203_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112203_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:34:07.67 -30:47:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.285 5632204234036137600 143.53203121597 -30.79584303704 13.9959 13.3689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112207_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112207_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:23:19.80 -32:00:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 0.944 5631248586636126592 140.83267880123 -32.01267496035 13.6845 13.3069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112215_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112215_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:31:31.32 -35:36:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.891 5437171899430815360 142.88052277091 -35.61014218969 13.4816 13.2167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112221_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112221_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:00:23.88 -33:59:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.172 5627674005614753920 135.09924998840 -33.99468350615 13.0305 12.0043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112228_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112228_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:06:54.04 -29:42:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.792 5635375122492091904 136.72525855123 -29.70156617895 13.4774 12.8453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112237_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112237_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:49:39.83 -33:03:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 4.661 5438790655423902720 147.41537982803 -33.06375613422 13.6238 13.0607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112238_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112238_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:46:19.22 -33:19:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.904 5438585527786396544 146.58096330898 -33.32884128490 13.3426 12.8599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112239_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112239_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:42:00.64 -30:05:44.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112242_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112242_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:32:02.25 -31:12:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.942 5632099673054439040 143.00966706011 -31.21185580060 13.0644 12.5682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112243_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112243_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:09:57.79 -29:55:21.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112246_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112246_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:25:22.83 -29:57:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.632 5633264468185083008 141.34548530374 -29.95772700920 12.6073 11.7138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112249_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112249_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:56:31.89 -30:26:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.192 5641480263888584832 134.13323495499 -30.44605961311 12.7081 12.1997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112251_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112251_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:18:24.63 -32:27:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.827 5630894883189523200 139.60321043726 -32.46550540097 12.4178 11.3157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112252_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112252_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:54:24.45 -29:49:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.252 5641747342133974144 133.60179466325 -29.82693686206 12.2144 11.3335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112255_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112255_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:44:51.52 -37:41:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.269 5433142498552995456 146.21474062808 -37.69028666561 11.6593 10.9039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112256_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112256_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:43:06.92 -29:39:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 1.239 5632572875371188224 145.77921188627 -29.65104551923 12.4301 11.8931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112257_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112257_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:37:50.11 -36:14:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 2.042 5436509611173618560 144.45849725496 -36.24306815549 10.3639 9.6941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112321_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112321_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:52:06.07 -33:05:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112325_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112325_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:51:34.11 -37:29:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.443 5625163476974572288 132.89247135259 -37.49015273928 11.2991 10.4927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112393_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112393_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:52:41.41 -29:42:58.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112577_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112577_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:52:33.20 -36:33:14.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112586_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112586_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:30:32.82 -32:05:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.267 5630532151729836416 142.63744005872 -32.09234488157 13.2312 12.7212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112590_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112590_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:35:57.79 -30:00:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.544 5632678501504940288 143.99096608774 -30.00786816340 13.4481 13.1602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112668_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112668_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:36:56.05 -34:14:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 0.771 5437732027587227776 144.23380078863 -34.23530720216 14.1966 12.9671 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112716_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112716_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:59:03.59 -31:15:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.584 5629282007011325184 134.76527324407 -31.26243144668 13.6092 13.0895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112765_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112765_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:24:29.32 -36:56:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.537 5431042431344546944 141.12165442765 -36.93926762185 13.6966 13.2054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112770_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112770_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:51:25.27 -31:54:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.237 5439149164933015040 147.85562822547 -31.90721863524 13.7014 13.2417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112776_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112776_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:27:04.27 -37:11:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.086 5430967733273085696 141.76856335655 -37.19531966295 13.8850 13.3526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112780_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112780_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:41:06.22 -30:07:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.890 5632529655117853184 145.27583161992 -30.11695840482 14.0133 13.2092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112798_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112798_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:47:55.32 -32:11:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.260 5439080338081434112 146.98073392174 -32.19006650828 13.6462 12.9251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112803_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112803_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:50:34.32 -32:21:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.345 5439109341996423424 147.64318734148 -32.36400524020 13.8989 13.4651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112816_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112816_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:51:48.77 -31:40:50.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112823_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112823_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:18:59.73 -34:24:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.899 5629813242925411456 139.74973222416 -34.40789266424 12.0152 10.5153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112825_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112825_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:38:11.45 -33:39:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.507 5439296568213146368 144.54776424687 -33.65879961042 14.1751 13.9880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112829_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112829_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:43:09.28 -36:49:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.663 5433428405935130880 145.78924287265 -36.82092016426 13.6610 13.1084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112830_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112830_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:29:59.25 -32:01:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.174 5630534969228401536 142.49725008941 -32.02879101155 14.0029 13.5149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112839_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112839_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112842_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112842_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:26:59.99 -38:14:27.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112846_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112846_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:00:47.04 -38:05:08.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112849_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112849_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:18:30.32 -36:07:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.587 5623376255180669312 139.62569210818 -36.13213708110 13.9188 13.4532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112874_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112874_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:56:04.99 -33:11:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.822 5628536744285740160 134.02139644932 -33.18622256542 13.6690 13.1930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112896_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112896_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:40:46.28 -30:10:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.353 5632527559173832320 145.19326543061 -30.17820959172 13.9597 13.4378 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112902_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112902_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:01:09.92 -35:56:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.047 5624223463250739200 135.29146792241 -35.94207519839 13.5772 12.8221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112908_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112908_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:47:58.91 -30:01:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.527 5464332001297788672 146.99554705910 -30.02456906872 13.8288 13.2546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112916_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112916_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:33:01.39 -33:19:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.044 5438078962166108160 143.25612761471 -33.32151767240 13.7942 13.2683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112922_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112922_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:55:27.29 -34:41:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.279 5626049167948334464 133.86394280809 -34.69920150150 13.3585 12.3472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112923_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112923_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112929_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112929_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:41:41.36 -35:48:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.258 5436628156571297280 145.42333685897 -35.81310375690 13.5762 12.7893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112946_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112946_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:41:04.81 -30:23:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.579 5632477290876830464 145.27077076904 -30.39840671114 14.0009 13.4918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112947_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112947_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:52:55.00 -34:21:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.075 5626867616917143936 133.22948602873 -34.36566530547 13.7896 12.9152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112950_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112950_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:47:17.70 -30:16:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.137 5464298569272683264 146.82411472456 -30.26949470850 13.6966 13.0523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112969_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112969_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:57:15.19 -37:18:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 3.369 5622495855605137280 134.31379822058 -37.30534477753 13.9597 13.1005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112971_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112971_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:58:29.08 -32:16:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.677 5629012042547032576 134.62084520699 -32.27889953257 13.9401 13.4463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112978_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112978_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:35:49.37 -30:19:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.420 5632620021230307456 143.95616393753 -30.32466577658 13.9416 13.4380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112980_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112980_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:19:08.47 -29:49:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.504 5634817979334265088 139.78597553676 -29.83258545952 14.1167 13.6603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112982_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112982_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:43:27.85 -31:01:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.541 5440184183331155968 145.86624149156 -31.03192019705 14.0839 13.5731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112987_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112987_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:46:15.27 -30:58:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 0.975 5440243934914793728 146.56380563473 -30.96994449873 13.7946 13.1276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112992_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 112992_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:26:39.56 -34:34:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 2.270 5629675529094246528 141.66546731780 -34.56997985914 14.2964 13.6837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113000_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113000_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:43:00.77 -30:35:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.372 5440303205465092736 145.75328480073 -30.58975350567 13.9653 13.4135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113008_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113008_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:59:07.69 -32:28:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.210 5628959128548782464 134.78204878822 -32.48272468368 13.8940 13.1703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113014_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113014_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:13:23.15 -36:16:53.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113017_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113017_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:37:33.11 -31:57:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.394 5439746199747102464 144.38790272535 -31.95068995355 14.1318 13.6308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113022_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113022_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:41:22.27 -30:35:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 3.640 5632366205842767872 145.34393901556 -30.59039519784 13.9278 13.2152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113028_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113028_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:16:03.44 -36:56:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.815 5623324956090962560 139.01481826583 -36.94364998386 13.9852 13.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113037_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113037_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:13:03.39 -33:07:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 3.305 5630930587257654272 138.26521457198 -33.12668537803 13.9479 13.4081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113040_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113040_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:35:26.38 -35:10:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.985 5437571297030095232 143.85973730289 -35.18173949401 13.3664 12.2030 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113048_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113048_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:11:23.68 -30:21:38.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113082_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113082_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:16:57.63 -36:42:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 2.437 5623334301939658624 139.24096903678 -36.71130071863 14.0397 13.2933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113094_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113094_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:58:20.96 -30:19:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.639 5641474147854954880 134.58806395536 -30.33212359782 13.8887 13.3938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113099_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113099_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:01:27.55 -32:23:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.646 5628972013451394816 135.36531329373 -32.38487245764 13.9071 13.3606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113122_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 113122_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 08:56:42.37 -33:46:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 3.172 5627659746325204864 134.17750050512 -33.76795776596 13.9395 13.5723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46823_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 46823_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105450_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 105450_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:19:38.14 -38:03:33.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38099_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 38099_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:00:35.79 -34:56:56.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81020_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 81020_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:37:34.78 -31:02:27.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104922_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 104922_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:28:58.57 -34:21:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 1.903 5437903590060327808 142.24466988927 -34.35781372356 11.1413 9.7278 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29908_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
Preparing report for the candidate 29908_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90155_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 90155_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:32:40.72 -32:03:04.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23403_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
Preparing report for the candidate 23403_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41859_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 41859_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:33:42.38 -34:43:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68300_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 68300_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:35:22.97 -29:44:06.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32836_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
Preparing report for the candidate 32836_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41004_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 41004_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23657_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 23657_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:22:04.49 -36:42:08.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78643_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 78643_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks
**** FOUND 09:02:42.70 -30:32:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 5.339 5635412540248706176 135.67665475248 -30.54535189983 10.9238 9.4823 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12889_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
Preparing report for the candidate 12889_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71653_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116
The candidate 71653_fd_Pyx-02-Q2b1x1_2026-03-20_22-41-24_20.00sec_-15.00C_LIGHT_0116 did not pass the final checks