This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 29.3652 2461128.8652 11.21 15:20:21.68 -37:35:16.4
332.92717 16.46190 galactic Lup Second-epoch detections are separated by 0.5" and 7.8 pix
The object was found in VSX 1" FM Lup
Type: SRA
# Max. Min./Amp. JD0 Period
10.000 V 14.700 V 2453113.00000 162.000000000000 Me
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FM Lup,2461128.8652,11.21,0.05,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
FM Lup 20260329.3652 11.21CV 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/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:20:21.68 -37:35:16.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20_00sec_-15_00C_LIGHT_0322_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20_00sec_-14_90C_LIGHT_0321_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20_00sec_-15_00C_LIGHT_0322_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20_00sec_-14_90C_LIGHT_0321_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3652 2461128.8652 12.37 16:05:26.66 -30:41:42.3
344.97829 15.92147 galactic Lup Second-epoch detections are separated by 0.5" and 8.6 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 6037026170378379392 | 16:05:26.87 -30:41:39.9 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037026170378379392,2461128.8652,12.37,0.05,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 6037026170378379392 20260329.3652 12.37CV 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/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:05:26.66 -30:41:42.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20_00sec_-15_00C_LIGHT_0322_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20_00sec_-14_90C_LIGHT_0321_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20_00sec_-15_00C_LIGHT_0322_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png resample_wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20_00sec_-14_90C_LIGHT_0321_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: 2461083.97781113 12.02.2026 11:27:52.882 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
First image: 2461083.97781113 12.02.2026 11:27:52.882 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
Last image: 2461128.86551747 29.03.2026 08:46:10.709 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.61
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: 4 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): 5519
Objects passed selection criteria: 5516
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 5266.5
Average stars matched: 4758.25 (90.3494 %)
Memory usage VmPeak: 112380 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 03:48:09 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: 2461083.97781113 12.02.2026 11:27:52.882 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
First image: 2461083.97781113 12.02.2026 11:27:52.882 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
Last image: 2461128.86551747 29.03.2026 08:46:10.709 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 211
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.27
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: 16 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): 51681
Objects passed selection criteria: 51610
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 50116.2
Average stars matched: 42283 (84.3698 %)
Memory usage VmPeak: 157420 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 03:49:04 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/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
SExtractor catalog cache: saved Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat to cache
SExtractor catalog cache: saved Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.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/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461128.86488216
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_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits exists and is non-empty
Saving wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits to local_wcs_cache/
'wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits' -> 'local_wcs_cache/wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits'
wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits exists and is non-empty
Saving wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits to local_wcs_cache/
'wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits' -> 'local_wcs_cache/wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits'
wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits exists and is non-empty
Saving wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits to local_wcs_cache/
'wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits' -> 'local_wcs_cache/wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits'
wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits exists and is non-empty
Saving wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits to local_wcs_cache/
'wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits' -> 'local_wcs_cache/wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:39:05.829 -34:00:17.24
Second-epoch image center 15:39:03.860 -33:59:20.09
Angular distance between the image centers 0.02 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 15:39:05.829 -34:00:17.24
Second-epoch image center 15:39:05.837 -34:00:01.99
Angular distance between the image centers 0.00 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 15:39:03.860 -33:59:20.09
Second-epoch second image center 15:39:05.837 -34:00:01.99
Angular distance between the image centers 0.01350 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/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits &> /tmp/tmp.Tjhaow1jTR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits &> /tmp/tmp.udxKMKtSKd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits &> /tmp/tmp.LgRNN9wmFG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits &> /tmp/tmp.2JTgDbi8hB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
Calibrating the magnitude scale
Found non-empty wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.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_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.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_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat
Found non-empty wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat
The reference image (wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits) and catalog (wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat) found
'wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.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 5497 out of 6767 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.671938
a=0.000000 b=1.000000 c=22.671938
From vast_summary.log: estimated ref. image limiting mag.: -8.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.06
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.06
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.6 pix Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
2.1 pix Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
2.8 pix fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
2.8 pix fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
Limiting magnitude estimates:
14.1 mag. Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
14.3 mag. Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
13.7 mag. fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
13.7 mag. fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.0 (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.Tjhaow1jTR (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits' -> 'wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
Checking if the catalog wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
WCS catalog name: wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=448, passed=6767
Got 6767 stars (including 6314 good ones) from the SExtractor catalog wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 6767 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits -region wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.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.udxKMKtSKd (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/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits' -> 'wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
WCS-calibrated image found: wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
Checking if the catalog wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat corresponding to the image wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat corresponding to the image wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
WCS catalog name: wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=636, passed=7483
Got 7483 stars (including 6835 good ones) from the SExtractor catalog wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat
util/solve_plate_with_UCAC5 got 7483 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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits -region wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.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.LgRNN9wmFG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
Checking if the catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat corresponding to the image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat corresponding to the image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
WCS catalog name: wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=321, passed=5267
Got 5267 stars (including 4943 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat
util/solve_plate_with_UCAC5 got 5267 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 959 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits -region wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.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.2JTgDbi8hB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
Checking if the catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
WCS catalog name: wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=355, passed=5264
Got 5264 stars (including 4902 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat
util/solve_plate_with_UCAC5 got 5264 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 957 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits -region wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.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_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits'
Saving fully-calibrated image wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits'
Saving fully-calibrated image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits'
Saving fully-calibrated image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits'
Preparing the HTML report for the field Lup-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21991.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21931_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 21931_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:10:45.14 -31:07:53.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21956_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 21956_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:16:11.23 -30:34:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21967_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 21967_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:10:15.33 -29:35:00.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21980_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 21980_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:16.95 -33:18:34.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21988_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 21988_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:13:16.38 -29:46:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 0.594 6211431838632736896 228.31842299746 -29.77979283480 10.9648 10.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21989_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 21989_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:34:56.02 -37:09:00.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21991_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 21991_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:20:21.68 -37:35:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 0.803 6007531186834374528 230.09019363101 -37.58775080243 10.4369 9.2134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21474_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 21474_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:15:25.21 -35:46:54.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Lup-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
SExtractor catalog cache: saved Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat to cache
SExtractor catalog cache: saved Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
Creating symlink local_wcs_cache/wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
Creating symlink local_wcs_cache/wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
Creating symlink local_wcs_cache/wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.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_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits exists and is non-empty
wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits exists and is non-empty
wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits exists and is non-empty
wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:39:05.829 -34:00:17.24
Second-epoch image center 15:39:03.860 -33:59:20.09
Angular distance between the image centers 0.02 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 15:39:05.829 -34:00:17.24
Second-epoch image center 15:39:05.837 -34:00:01.99
Angular distance between the image centers 0.00 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 15:39:03.860 -33:59:20.09
Second-epoch second image center 15:39:05.837 -34:00:01.99
Angular distance between the image centers 0.01350 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/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits &> /tmp/tmp.9ti9JBMLSm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits &> /tmp/tmp.pHIfyorFcn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits &> /tmp/tmp.hOapm4Vt9G
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits &> /tmp/tmp.VVcsqf5uZN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
Calibrating the magnitude scale
Found non-empty wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.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_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.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_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat
Found non-empty wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat
The reference image (wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits) and catalog (wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat) found
'wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.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 8469 out of 56189 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.419086
a=0.000000 b=1.000000 c=22.419086
From vast_summary.log: estimated ref. image limiting mag.: -8.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.15
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 86 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
1.9 pix Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
2.5 pix fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
2.4 pix fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
Limiting magnitude estimates:
14.1 mag. Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
14.4 mag. Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
13.9 mag. fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
13.9 mag. fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
All-image limiting magnitude estimate: 13.9 (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.9ti9JBMLSm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits' -> 'wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
Checking if the catalog wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
WCS catalog name: wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2994, passed=56185
Got 56185 stars (including 53132 good ones) from the SExtractor catalog wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 56185 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 959 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: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits -region wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.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.pHIfyorFcn (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/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits' -> 'wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
WCS-calibrated image found: wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
Checking if the catalog wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat corresponding to the image wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat corresponding to the image wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
WCS catalog name: wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=4169, passed=80037
Got 80037 stars (including 75708 good ones) from the SExtractor catalog wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat
util/solve_plate_with_UCAC5 got 80037 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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits -region wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.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.hOapm4Vt9G (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
Checking if the catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat corresponding to the image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat corresponding to the image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
WCS catalog name: wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1873, passed=43261
Got 43261 stars (including 41343 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat
util/solve_plate_with_UCAC5 got 43261 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 958 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits -region wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.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.VVcsqf5uZN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
Checking if the catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
WCS catalog name: wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1994, passed=44751
Got 44751 stars (including 42695 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat
util/solve_plate_with_UCAC5 got 44751 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 955 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits -region wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.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_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/wcs_Lup-01-Q2b1x1_2026-02-12_05-27-52_20.00sec_-14.90C_LIGHT_0025.fits
Saving fully-calibrated image wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/wcs_Lup-01-Q2b1x1_2026-02-27_06-18-16_20.00sec_-14.90C_LIGHT_0071.fits
Saving fully-calibrated image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-45-15_20.00sec_-14.90C_LIGHT_0321.fits
Saving fully-calibrated image wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Lup-01-Q2b1x1_034647_TTUQ2b1x1_22469_3fHnrPfm/wcs_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322.fits
Preparing the HTML report for the field Lup-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out95571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44092.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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 95569_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95569_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 16:02:58.21 -31:54:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95571_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95571_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:47:38.41 -31:49:07.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 95572_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95572_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:13:13.87 -32:35:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.882 6207467618177197312 228.30822248436 -32.59995961287 13.3857 12.6709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95574_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95574_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:06:43.76 -35:19:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.506 6200764892216377472 226.68250484806 -35.32326252738 12.7962 12.0312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95575_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95575_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:11:24.80 -31:38:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 0.937 6210596793911075200 227.85363737049 -31.63666609368 12.9703 12.2270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95578_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95578_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:29:00.77 -36:36:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.218 6013472500994602624 232.25337779566 -36.60330129801 12.3507 11.4366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95579_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95579_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:08:17.30 -35:07:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.162 6200608825985204992 227.07241809196 -35.12741235810 12.8387 12.2887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95585_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95585_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:10:03.18 -34:16:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.019 6201223934022062848 227.51349252725 -34.28000390009 12.1920 11.2828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95590_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95590_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:23.74 -37:25:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95679_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95679_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:18:44.52 -36:33:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95758_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95758_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:09:12.69 -35:12:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 2.232 6200593398462682112 227.30332106136 -35.20897055962 11.9866 11.2614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95771_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95771_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:12:43.33 -29:58:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95775_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95775_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:56:14.34 -31:45:07.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 95819_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95819_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:16:54.70 -30:22:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.423 6211141082229194240 229.22833880316 -30.37562396685 12.0969 11.2534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95826_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95826_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:12:15.40 -31:10:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95847_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95847_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:12:27.44 -35:55:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 0.177 6200121295659006848 228.11434104582 -35.92699322664 12.3898 11.7006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95884_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95884_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:14:41.27 -30:51:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.578 6210739558623360640 228.67181448146 -30.86194061209 12.7616 12.0112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95885_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95885_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:08:23.02 -30:35:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95902_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95902_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:08:35.46 -29:48:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95907_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95907_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:45.67 -33:39:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.706 6204315520200642432 226.94088650527 -33.65643080306 12.7499 11.9725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95922_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95922_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:13.43 -34:15:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.971 6201259912966104960 226.80600681888 -34.25237978267 13.1347 12.5022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95943_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95943_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:11.39 -34:53:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95954_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95954_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:08:19.19 -31:52:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.919 6210752301788161536 227.08020078094 -31.87076586421 12.7226 11.9699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 95981_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95981_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 95983_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95983_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:08:30.08 -30:14:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95992_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 95992_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:10:18.55 -29:57:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96000_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96000_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:53.75 -30:35:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.968 6211641325658312192 226.97427066891 -30.59688632638 13.1332 12.4485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96002_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96002_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:10:43.93 -31:10:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.984 6210892493819715712 227.68333372538 -31.16841673891 12.9447 12.1543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96018_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96018_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:10:56.56 -31:34:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96020_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96020_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:08:00.69 -30:51:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96021_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96021_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:09:40.55 -31:07:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.159 6210815046969160192 227.41860081240 -31.12306663752 13.0944 12.3188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96027_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96027_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:12:38.23 -31:57:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96031_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96031_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:11:12.53 -29:32:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96035_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96035_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:08:30.45 -31:55:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96036_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96036_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:07.77 -31:59:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96037_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96037_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:15:38.22 -30:34:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96040_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96040_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:10:55.93 -31:11:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96044_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96044_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:14:13.14 -30:49:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96049_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96049_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:10:00.51 -31:31:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96055_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96055_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:17:14.03 -34:34:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.410 6200310484677437184 229.30971006871 -34.56598965840 12.9168 11.8868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96057_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96057_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:16.52 -30:29:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.367 6211655486170908032 226.81891149656 -30.49126526221 12.9413 12.1675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96062_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96062_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:09:44.65 -31:10:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.080 6210813805719842944 227.43613415398 -31.17609425899 13.1829 12.4477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96063_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96063_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:11:56.86 -31:22:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.974 6210699254649962624 227.98661632729 -31.36785788759 13.1758 12.4128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96068_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96068_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:09:21.40 -30:23:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96079_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96079_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:06:43.52 -32:18:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.435 6204733441997611392 226.68171039352 -32.31170494323 13.0665 12.4650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96081_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96081_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:13:10.87 -31:45:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96086_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96086_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:15:19.74 -30:03:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.937 6211351643003176320 228.83234808908 -30.06022632520 13.1620 12.4939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96091_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96091_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:09:37.30 -30:36:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.808 6210984268681219200 227.40591546991 -30.60904472836 13.5113 12.7599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96092_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96092_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:12:18.82 -30:54:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96096_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96096_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:05:57.16 -35:12:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96103_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96103_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:13:03.20 -31:54:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96110_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96110_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:38.64 -32:17:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.089 6204731724010392704 226.91161804099 -32.28633072007 13.1421 12.3703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96113_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96113_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:13:53.99 -31:50:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.234 6210612423292901248 228.47566565800 -31.84315068534 13.4283 12.8364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96115_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96115_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:08:51.97 -33:02:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.650 6204429049075532544 227.21706865157 -33.04721129629 13.0741 12.3383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.650#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96116_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96116_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:35.49 -31:35:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96117_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96117_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:06:34.32 -34:34:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96120_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96120_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:13:53.65 -30:48:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.414 6210744265907582976 228.47386533487 -30.80894489594 13.0761 12.4360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96124_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96124_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:12:42.23 -31:58:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.673 6210527249800488704 228.17648910307 -31.97027404614 13.3928 12.7561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96138_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96138_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:15:52.62 -31:34:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.555 6210642458002631040 228.96961004712 -31.58316538235 13.3554 12.9926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96153_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96153_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:06:44.91 -34:31:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.861 6200871441765412096 226.68775242644 -34.52756447227 13.3515 12.8605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96162_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96162_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:08:33.96 -33:04:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.890 6204439185198348800 227.14179453968 -33.07779287097 13.4438 12.8620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96180_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96180_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:16:15.66 -31:58:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.965 6207595947501957376 229.06550673832 -31.97212137558 13.2149 12.4115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.965#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96195_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96195_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:06:35.83 -33:14:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96196_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96196_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:15:47.66 -31:28:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.179 6210647130927068032 228.94874328928 -31.46989678125 13.5751 12.9903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96197_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96197_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:06:45.82 -34:16:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.325 6201265612384692224 226.69202547850 -34.27278273898 13.5098 12.9153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96217_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96217_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:13:13.50 -34:51:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96226_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96226_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:06:53.79 -33:13:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.586 6204341156864935424 226.72439996811 -33.22476322798 13.0390 12.1031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96246_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96246_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:07:03.26 -35:10:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96272_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96272_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:34:34.88 -35:16:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96283_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96283_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:05:22.04 -35:27:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 2.157 6200759184201547264 226.34256714849 -35.46134830283 13.4320 12.9152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96323_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 96323_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:36:45.75 -31:12:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.765 6208462092087524608 234.19108277771 -31.20592729204 13.5891 11.9675 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07855_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 07855_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:36:55.14 -37:46:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07402_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 07402_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:04:35.95 -37:08:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76505_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 76505_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:56:03.33 -32:12:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07408_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
Preparing report for the candidate 07408_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
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Considering the candidate 44092_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
Preparing report for the candidate 44092_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
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Considering the candidate 12552_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 12552_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:05:22.39 -36:15:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38000_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 38000_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:10:45.17 -31:07:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70421_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 70421_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:34:26.67 -31:10:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21756_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 21756_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:54:30.63 -35:24:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72956_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 72956_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:56:47.02 -30:41:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72063_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 72063_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:34:56.01 -37:09:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75949_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 75949_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:28:35.43 -37:33:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43222_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 43222_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:10:15.37 -29:35:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16637_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 16637_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks
**** FOUND 15:15:25.23 -35:46:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77700_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322
The candidate 77700_fd_Lup-01-Q2b1x1_2026-03-29_03-46-10_20.00sec_-15.00C_LIGHT_0322 did not pass the final checks