This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IK Gem,2461129.7516,9.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IK Gem 20260330.2516 9.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:37:40.79 +27:36:24.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20_00sec_-10_00C_LIGHT_0237_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20_00sec_-10_00C_LIGHT_0236_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20_00sec_-10_00C_LIGHT_0237_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20_00sec_-10_00C_LIGHT_0236_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461129.7516,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.2516 13.24CV 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/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:39:52.85 +25:59:17.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20_00sec_-10_00C_LIGHT_0237_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20_00sec_-10_00C_LIGHT_0236_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20_00sec_-10_00C_LIGHT_0237_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20_00sec_-10_00C_LIGHT_0236_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461129.7516,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.2516 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:08:20.78 +31:13:37.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20_00sec_-10_00C_LIGHT_0237_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20_00sec_-10_00C_LIGHT_0236_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20_00sec_-10_00C_LIGHT_0237_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20_00sec_-10_00C_LIGHT_0236_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.2516 2461129.7516 9.83 06:36:05.10 +27:46:07.1
186.35492 9.19119 galactic Gem Second-epoch detections are separated by 0.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3385999972463251072 | 06:36:04.88 +27:46:14.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3385999972463251072,2461129.7516,9.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3385999972463251072 20260330.2516 9.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:05.10 +27:46:07.1 ;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_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20_00sec_-10_00C_LIGHT_0237_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20_00sec_-10_00C_LIGHT_0236_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20_00sec_-10_00C_LIGHT_0237_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20_00sec_-14_90C_LIGHT_0226_fits__*pix.png resample_wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20_00sec_-10_00C_LIGHT_0236_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.73602979 18.01.2026 05:39:42.974 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
First image: 2461058.73602979 18.01.2026 05:39:42.974 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Last image: 2461129.75188177 30.03.2026 06:02:32.585 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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: 6 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): 20446
Objects passed selection criteria: 20291
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 12904.5
Average stars matched: 12400.5 (96.0944 %)
Memory usage VmPeak: 125468 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Mar 30 01:04:42 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: 2461058.73602979 18.01.2026 05:39:42.974 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
First image: 2461058.73602979 18.01.2026 05:39:42.974 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Last image: 2461129.75188177 30.03.2026 06:02:32.585 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 72
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 112 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): 142489
Objects passed selection criteria: 142083
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 96745.5
Average stars matched: 92044.8 (95.1411 %)
Memory usage VmPeak: 1906072 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Mar 30 01:08:35 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/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
SExtractor catalog cache: saved Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.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/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.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: 2461129.75124553
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits'
wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits'
wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits exists and is non-empty
Saving wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits to local_wcs_cache/
'wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits' -> 'local_wcs_cache/wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits'
wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits exists and is non-empty
Saving wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits to local_wcs_cache/
'wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits' -> 'local_wcs_cache/wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.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 07:00:00.353 +29:59:44.05
Second-epoch image center 06:59:59.510 +29:59:35.45
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:00:00.353 +29:59:44.05
Second-epoch image center 07:00:00.150 +30:00:13.48
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 06:59:59.510 +29:59:35.45
Second-epoch second image center 07:00:00.150 +30:00:13.48
Angular distance between the image centers 0.01081 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/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits &> /tmp/tmp.guIjuzYPAq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits &> /tmp/tmp.hUglAWRYY2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits &> /tmp/tmp.OEPXu2wIxE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits &> /tmp/tmp.8VsCxXYsip
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat
Found non-empty wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat
The reference image (wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits) and catalog (wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat) found
'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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 11962 out of 24243 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.882669
a=0.000000 b=1.000000 c=22.882669
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
2.1 pix Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
2.4 pix fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
2.4 pix fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
Limiting magnitude estimates:
15.3 mag. Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
15.3 mag. Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
13.5 mag. fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
13.5 mag. fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.guIjuzYPAq (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/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits' -> 'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Checking if the catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS catalog name: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2293, passed=24243
Got 24243 stars (including 21925 good ones) from the SExtractor catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 24243 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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 942 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 - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits -region wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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.hUglAWRYY2 (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/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits' -> 'wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Checking if the catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS catalog name: wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2282, passed=24037
Got 24037 stars (including 21723 good ones) from the SExtractor catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 24037 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits -region wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.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.OEPXu2wIxE (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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
WCS-calibrated image found: wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
Checking if the catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
WCS catalog name: wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=427, passed=5660
Got 5660 stars (including 5225 good ones) from the SExtractor catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat
util/solve_plate_with_UCAC5 got 5660 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 940 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits -region wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.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.8VsCxXYsip (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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
WCS_IMAGE_NAME=wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
WCS-calibrated image found: wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
Checking if the catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
WCS catalog name: wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=411, passed=5614
Got 5614 stars (including 5202 good ones) from the SExtractor catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat
util/solve_plate_with_UCAC5 got 5614 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 936 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits -region wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.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_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits'
Saving fully-calibrated image wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits'
Saving fully-calibrated image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits'
Preparing the HTML report for the field Gem-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out08118.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
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 31610_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 31610_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:33:17.71 +31:35:29.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19966_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 19966_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:26:13.06 +33:22:17.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08118_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
Preparing report for the candidate 08118_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13804_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 13804_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:47:07.12 +30:16:34.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Gem-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:37:40.79 +27:36:24.9
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/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
SExtractor catalog cache: saved Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.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_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits exists and is non-empty
wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits exists and is non-empty
wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits exists and is non-empty
wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.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 07:00:00.353 +29:59:44.05
Second-epoch image center 06:59:59.510 +29:59:35.45
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:00:00.353 +29:59:44.05
Second-epoch image center 07:00:00.150 +30:00:13.48
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 06:59:59.510 +29:59:35.45
Second-epoch second image center 07:00:00.150 +30:00:13.48
Angular distance between the image centers 0.01081 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/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits &> /tmp/tmp.ecjSzCYxIq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits &> /tmp/tmp.F1iv8MS5AL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits &> /tmp/tmp.dcdTR3Vr9D
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits &> /tmp/tmp.FBURUXcpye
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat
Found non-empty wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits and wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat
The reference image (wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits) and catalog (wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat) found
'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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 12230 out of 167542 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.731957
a=0.000000 b=1.000000 c=22.731957
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 57 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
1.9 pix Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
2.1 pix fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
2.2 pix fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
Limiting magnitude estimates:
15.5 mag. Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
15.5 mag. Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
13.8 mag. fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
13.7 mag. fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ecjSzCYxIq (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/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits' -> 'wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Checking if the catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
WCS catalog name: wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=20873, passed=167504
Got 167504 stars (including 146353 good ones) from the SExtractor catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 167504 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 935 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: 0.41"
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 935 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: 0.43"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits -region wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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.F1iv8MS5AL (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/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits' -> 'wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Checking if the catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
WCS catalog name: wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=20907, passed=166940
Got 166940 stars (including 145746 good ones) from the SExtractor catalog wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 166940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 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: 0.43"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits -region wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.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.dcdTR3Vr9D (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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
WCS-calibrated image found: wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
Checking if the catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
WCS catalog name: wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1877, passed=47483
Got 47483 stars (including 45551 good ones) from the SExtractor catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat
util/solve_plate_with_UCAC5 got 47483 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 938 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits -region wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.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.FBURUXcpye (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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
WCS_IMAGE_NAME=wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
WCS-calibrated image found: wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
Checking if the catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat corresponding to the image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
WCS catalog name: wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1812, passed=46604
Got 46604 stars (including 44738 good ones) from the SExtractor catalog wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat
util/solve_plate_with_UCAC5 got 46604 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 938 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: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 935 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits -region wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.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_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/wcs_Gem-01-Q2b1x1_2026-01-17_23-39-42_20.00sec_-14.90C_LIGHT_0226.fits
Saving fully-calibrated image wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/wcs_Gem-01-Q2b1x1_2026-01-17_23-40-27_20.00sec_-15.00C_LIGHT_0227.fits
Saving fully-calibrated image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-01-37_20.00sec_-10.00C_LIGHT_0236.fits
Saving fully-calibrated image wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.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_2026-03-30_CI_Gem-01-Q2b1x1_010314_TTUQ2b1x1_28307_SxPlYAts/wcs_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237.fits
Preparing the HTML report for the field Gem-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out178640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out190863.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out195333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58256.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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
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Considering the candidate 190856_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 190856_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:26:30.98 +28:48:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.427 873528251300900224 111.62914755097 +28.80738533559 12.9582 12.4147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190857_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 190857_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:25:19.60 +28:10:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.588 873062642486542208 111.33123386929 +28.17163822305 13.0783 12.6182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190863_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 190863_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:43:17.70 +26:58:58.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)
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Considering the candidate 190864_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 190864_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:43:29.88 +26:58:14.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)
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Considering the candidate 190867_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 190867_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:12:23.45 +26:48:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.490 883391935754719616 108.09781170780 +26.81492778694 12.4237 11.9688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190869_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 190869_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:18:16.69 +31:52:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 2.395 887099519027049728 109.56943280799 +31.86609119285 12.6694 11.7370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190870_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 190870_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:16:21.40 +27:08:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.906 883439592711843840 109.08889676261 +27.13806408117 12.2593 11.8479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190871_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 190871_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:47:04.45 +26:33:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192063_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 192063_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:52:42.51 +33:55:49.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 192120_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 192120_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:50:21.94 +29:19:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 1.150 888417322369761920 102.59158582728 +29.32094993161 11.6485 10.9225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192533_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 192533_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:53:43.90 +29:29:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.350 888479303040350336 103.43282453339 +29.49708265926 12.1370 11.6376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193039_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193039_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:41:18.79 +29:41:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.949 3434721458697384448 100.32791459545 +29.69109667825 12.1786 11.7133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193184_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193184_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:54:52.19 +26:07:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193316_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193316_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:37:40.12 +28:25:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.346 3434175246233505536 099.41727483720 +28.42640264612 12.2456 11.8159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193351_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193351_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:45:39.19 +27:38:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.679 3386159642167713024 101.41309380382 +27.64809704537 12.3292 11.6356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193433_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193433_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:00:00.57 +29:47:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.199 888093477538114816 105.00199475929 +29.78671249216 12.4491 11.8147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193436_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193436_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:46:17.74 +27:48:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.710 3386186026150223488 101.57380585562 +27.81450436767 12.3791 11.7089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193444_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193444_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:39:34.06 +28:18:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.978 3386123491426054144 099.89198261716 +28.30534867603 12.4394 12.2443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193469_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193469_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:00:11.05 +29:45:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.756 888090213362971520 105.04581181610 +29.75006567239 12.4944 12.2277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193652_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193652_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:35:05.40 +28:00:00.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193657_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193657_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:35:16.92 +28:00:06.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193777_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193777_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:54:05.57 +32:29:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 1.073 937468116632253952 103.52292605768 +32.49073727433 12.4709 11.6922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193798_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193798_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:18:25.09 +27:14:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.763 883455604349864192 109.60447359280 +27.24054047703 12.8502 12.3913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193892_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193892_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:47:27.20 +30:37:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.310 936794906279010176 101.86230916287 +30.62326174136 12.8582 12.1487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193949_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193949_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:59:37.42 +26:03:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 0.533 3381842096226402432 104.90575184022 +26.05755602596 12.6785 12.0214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193972_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193972_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:06:39.64 +31:31:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.254 889794971783072896 106.66475847768 +31.52793182698 12.6120 11.9026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193978_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 193978_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:17:20.41 +26:22:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.733 871377812716086016 109.33551478691 +26.37458930515 12.7938 12.3781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194056_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 194056_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:59:26.43 +31:30:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.645 889146504737350400 104.85977362341 +31.49979383198 12.9368 12.1879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194098_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 194098_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:56:52.76 +33:40:03.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194169_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 194169_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:58:55.87 +26:10:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.838 3381894567843373312 104.73291041148 +26.18377713054 13.1756 12.6599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194298_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 194298_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:23:06.66 +29:16:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.102 885599067907876480 110.77735166563 +29.27466964878 12.9775 12.4432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194315_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 194315_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:10:49.34 +32:38:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 0.453 890334905008276096 107.70544152321 +32.63437294620 12.8497 12.0219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194349_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 194349_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:59:13.41 +26:25:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.305 3381916416340515456 104.80553497815 +26.42283559147 13.0367 12.4934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194486_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 194486_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:46:25.39 +26:07:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194644_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 194644_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:49:04.59 +27:12:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.459 3385342842467063424 102.26866956022 +27.20412459508 12.8748 12.5168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194685_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 194685_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:49:15.75 +27:12:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.044 3385342975608366464 102.31498687392 +27.20638116771 12.5594 11.7487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194751_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 194751_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:03:49.74 +33:53:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195024_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195024_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:13:12.59 +30:33:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.837 886538561938074496 108.30272611877 +30.55210950012 13.2191 12.7701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195142_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195142_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:14:05.73 +30:55:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.344 886573437073246976 108.52344059335 +30.92039592730 13.2907 12.6213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195307_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195307_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:55:58.74 +26:37:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.750 3382145737531975040 103.99525946973 +26.63303098062 13.7605 13.3648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195333_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
Preparing report for the candidate 195333_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
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Considering the candidate 195462_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195462_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:51:29.84 +26:40:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.455 3385077997604148864 102.87540094323 +26.67189614602 13.4681 13.0680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195479_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195479_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:47:31.39 +30:38:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.118 936795112437434112 101.88059003931 +30.64293689041 13.2188 12.6562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195554_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195554_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:06:22.79 +33:20:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.678 891223688360822784 106.59445895729 +33.33659747111 13.2416 12.5019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195558_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195558_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:11:39.67 +28:12:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.759 883795314787681280 107.91457057156 +28.21001192769 13.5474 13.1044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195598_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195598_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:49:13.66 +28:32:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.857 3386327386410274304 102.30657484855 +28.54466939429 13.4238 12.7521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195681_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195681_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:42:30.17 +32:31:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.544 938042474019769984 100.62595362977 +32.52448532219 13.3218 12.8457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195720_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195720_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:55:21.03 +30:56:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.223 889022324346010880 103.83733908769 +30.94201477326 13.3961 12.7465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195789_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195789_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 07:13:30.81 +32:10:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.514 890084697392904704 108.37828482861 +32.17334302321 13.7556 13.2158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195796_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 195796_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:33:47.28 +27:58:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.792 3434100307643942400 098.44658919895 +27.96857571712 13.2747 12.8066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195837_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
Preparing report for the candidate 195837_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
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Considering the candidate 178640_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 178640_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:56:15.99 +29:41:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.908 887763383533393920 104.06642759899 +29.68362074907 12.1233 11.3263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96257_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 96257_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:47:07.12 +30:16:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55671_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 55671_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:37:40.80 +27:36:24.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 146225_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 146225_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks
**** FOUND 06:33:17.73 +31:35:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58256_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
Preparing report for the candidate 58256_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
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Considering the candidate 127611_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237
The candidate 127611_fd_Gem-01-Q2b1x1_2026-03-30_01-02-32_20.00sec_-10.00C_LIGHT_0237 did not pass the final checks