This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh
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 06 04.2257 2461195.7258 12.29 16:43:04.42 -32:50:15.2
348.98456 8.62739 galactic Sco Second-epoch detections are separated by 1.6" and 8.2 pix
The object was found in VSX19" Gaia DR3 6027307479709696128
Type: E
# Max. Min./Amp. JD0 Period
18.480 G 19.010 G 0.964810000000
The object was found in astcheck.1048 Feodosia 5 -2 5 12.3 -0 -0
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:43:04.42 -32:50:15.2: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:43:04.42 -32:50:15.2: 14.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6027307479709696128,2461195.7258,12.29,0.05,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 6027307479709696128 20260604.2257 12.29CV 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
Mean magnitude and position on the discovery images:
2026 06 04.2257 2461195.7258 12.36 16:44:27.16 -31:00:33.9
350.59191 9.58075 galactic Sco Second-epoch detections are separated by 1.1" and 8.3 pix
The object was found in VSX 8" Gaia DR3 6030581069424775552
Type: ROT
# Max. Min./Amp. JD0 Period
14.890 G 14.930 G M
The object was found in astcheck.127 Johanna 2 1 2 12.5 -0 -0
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:44:27.16 -31:00:33.9: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:44:27.16 -31:00:33.9: 14.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030581069424775552,2461195.7258,12.36,0.05,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 6030581069424775552 20260604.2257 12.36CV 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
Mean magnitude and position on the discovery images:
2026 06 04.2257 2461195.7258 12.97 16:33:25.51 -30:01:00.6
349.78368 12.02932 galactic Sco Second-epoch detections are separated by 4.4" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.123 Brunhild 1 2 2 13.2 -0 -0
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:33:25.51 -30:01:00.6: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:33:25.51 -30:01:00.6: 14.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461195.7258,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260604.2257 12.97CV 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
Mean magnitude and position on the discovery images:
2026 06 04.2257 2461195.7258 13.09 16:11:45.14 -30:37:37.3
346.03293 15.02053 galactic Sco Second-epoch detections are separated by 2.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.195 Eurykleia -1 1 1 13.4 -0 -0
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:11:45.14 -30:37:37.3: 14.37 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:11:45.14 -30:37:37.3: 14.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461195.7258,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260604.2257 13.09CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461147.86060031 17.04.2026 08:39:05.867 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
First image: 2461147.86060031 17.04.2026 08:39:05.867 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Last image: 2461195.72604065 04.06.2026 05:25:19.912 /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.49
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4429
Objects passed selection criteria: 4428
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 4283.5
Average stars matched: 3960.5 (92.4594 %)
Memory usage VmPeak: 111316 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 1 15:05:05 CDT 2026
VaST build number 1.0rc89-85-g6dfb2809
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 4 00:52:23 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: 2461147.86060031 17.04.2026 08:39:05.867 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
First image: 2461147.86060031 17.04.2026 08:39:05.867 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Last image: 2461195.72604065 04.06.2026 05:25:19.912 /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 103
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.03
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: 71 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): 62577
Objects passed selection criteria: 62478
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 59302.8
Average stars matched: 54761.5 (92.3423 %)
Memory usage VmPeak: 168324 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 1 15:05:05 CDT 2026
VaST build number 1.0rc89-85-g6dfb2809
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 4 00:56:38 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/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
SExtractor catalog cache: saved Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat to cache
SExtractor catalog cache: saved Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.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/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.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: 2461195.72545878
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits exists and is non-empty
Saving wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits to local_wcs_cache/
'wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits' -> 'local_wcs_cache/wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits'
wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits exists and is non-empty
Saving wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits to local_wcs_cache/
'wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits' -> 'local_wcs_cache/wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits'
wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits exists and is non-empty
Saving wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits to local_wcs_cache/
'wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits' -> 'local_wcs_cache/wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits'
wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits exists and is non-empty
Saving wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits to local_wcs_cache/
'wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits' -> 'local_wcs_cache/wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits (1st reference image)
verification OK: wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Image size: 941.4'x627.4' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:41:52.558 -34:02:25.57 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits (1st new image)
verification OK: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
Image size: 937.5'x625.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:41:50.925 -34:05:21.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:41:52.558 -34:02:25.57
Second-epoch image center 16:41:50.925 -34:05:21.57
Angular distance between the image centers 0.0492 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits (2nd new image)
verification OK: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
Image size: 937.5'x625.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:41:48.700 -34:04:40.32 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:41:52.558 -34:02:25.57
Second-epoch image center 16:41:48.700 -34:04:40.32
Angular distance between the image centers 0.0397 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 16:41:50.925 -34:05:21.57
Second-epoch second image center 16:41:48.700 -34:04:40.32
Angular distance between the image centers 0.01379 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/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits &> /tmp/tmp.gXumUQ50R5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits &> /tmp/tmp.1S5JxxLq2e
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits &> /tmp/tmp.vHqNykoXPE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits &> /tmp/tmp.mCEztt7eQz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.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_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits and wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits and wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat
Found non-empty wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits and wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat
The reference image (wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits) and catalog (wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat) found
'wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat' -> 'wcsmag.cat'
Read 5944 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.0348 to 260.1069 deg, Dec -39.5112 to -28.0873 deg
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
Tycho-2 catalog search boundaries: RA 240.0348 to 260.1069 deg, Dec -39.5112 to -28.0873 deg
Loaded 14012 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4801 out of 4901 total matches.
Matched with Tycho-2 4901 out of 5944 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.247700
a=0.000000 b=1.000000 c=22.247700
From vast_summary.log: estimated ref. image limiting mag.: -8.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.76
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5944 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.0348 to 260.1069 deg, Dec -39.5112 to -28.0873 deg
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
Tycho-2 catalog search boundaries: RA 240.0348 to 260.1069 deg, Dec -39.5112 to -28.0873 deg
Loaded 14012 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4801 out of 4901 total matches.
Matched with Tycho-2 4901 out of 5944 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits:
Forced-photometry filter: calibrated wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits -> calib.txt_param_ref_wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits (aperture=6.2)
Read 7789 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.4677 to 260.4336 deg, Dec -39.2687 to -28.4832 deg
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
Tycho-2 catalog search boundaries: RA 240.4677 to 260.4336 deg, Dec -39.2687 to -28.4832 deg
Loaded 13342 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6087 out of 6270 total matches.
Matched with Tycho-2 6270 out of 7789 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits:
Forced-photometry filter: calibrated wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits -> calib.txt_param_ref_wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
2.4 pix Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
2.3 pix fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
2.3 pix fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
2.2 pix wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
2.4 pix wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
Limiting magnitude estimates:
13.8 mag. Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
13.9 mag. Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
13.6 mag. fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
13.5 mag. fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.8 (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.gXumUQ50R5 (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/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits' -> 'wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS-calibrated image found: wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Checking if the catalog wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS catalog name: wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=444, passed=5944
Got 5944 stars (including 5491 good ones) from the SExtractor catalog wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat
util/solve_plate_with_UCAC5 got 5944 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.5 to -28.1)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 5810 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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...
Searching UCAC5 zones 252 to 311 (Dec -39.5 to -28.1)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 956 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits N_match=956 sigma_overall_arcsec=0.546 sigma_q1_arcsec=0.494 sigma_q2_arcsec=0.499 sigma_q3_arcsec=0.551 sigma_q4_arcsec=0.616 n_q1=207 n_q2=194 n_q3=244 n_q4=311 worst_quadrant_to_overall_ratio=1.129
The image catalog is written to wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits -region wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1S5JxxLq2e (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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits' -> 'wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
WCS-calibrated image found: wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
Checking if the catalog wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
WCS catalog name: wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=575, passed=7789
Got 7789 stars (including 7202 good ones) from the SExtractor catalog wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat
util/solve_plate_with_UCAC5 got 7789 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...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 7649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 7648 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 7645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Excluding outliers - 957 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits N_match=957 sigma_overall_arcsec=0.825 sigma_q1_arcsec=0.642 sigma_q2_arcsec=1.084 sigma_q3_arcsec=0.706 sigma_q4_arcsec=0.843 n_q1=184 n_q2=235 n_q3=215 n_q4=323 worst_quadrant_to_overall_ratio=1.314
The image catalog is written to wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits -region wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.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.vHqNykoXPE (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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
Checking if the catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
WCS catalog name: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=521, passed=5752
Got 5752 stars (including 5224 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat
util/solve_plate_with_UCAC5 got 5752 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...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.6)
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...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
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...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5617 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5617 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits N_match=956 sigma_overall_arcsec=0.723 sigma_q1_arcsec=0.587 sigma_q2_arcsec=0.783 sigma_q3_arcsec=0.805 sigma_q4_arcsec=0.738 n_q1=173 n_q2=236 n_q3=221 n_q4=326 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits -region wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.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.mCEztt7eQz (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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
Checking if the catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
WCS catalog name: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=533, passed=5820
Got 5820 stars (including 5284 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat
util/solve_plate_with_UCAC5 got 5820 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...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.6)
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...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits N_match=956 sigma_overall_arcsec=0.754 sigma_q1_arcsec=0.660 sigma_q2_arcsec=0.856 sigma_q3_arcsec=0.851 sigma_q4_arcsec=0.784 n_q1=179 n_q2=230 n_q3=225 n_q4=322 worst_quadrant_to_overall_ratio=1.136
The image catalog is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits -region wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits sigma_overall=0.546 worst_q_ratio=1.129
ref2=Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits sigma_overall=0.825 worst_q_ratio=1.314
new1=fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits sigma_overall=0.723 worst_q_ratio=1.114
new2=fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits sigma_overall=0.754 worst_q_ratio=1.136
reference average sigma_overall=0.6855 worst_q_ratio=1.2215
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236_astrometric_residuals.png (956 matched stars from wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246_astrometric_residuals.png (957 matched stars from wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123_astrometric_residuals.png (956 matched stars from wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124_astrometric_residuals.png (956 matched stars from wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits'
Saving fully-calibrated image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits'
Preparing the HTML report for the field Sco-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Sco-03-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/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
SExtractor catalog cache: saved Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat to cache
SExtractor catalog cache: saved Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Creating symlink local_wcs_cache/wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.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_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits exists and is non-empty
wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits exists and is non-empty
wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits exists and is non-empty
wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits (1st reference image)
verification OK: wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Image size: 941.4'x627.4' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:41:52.558 -34:02:25.57 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits (1st new image)
verification OK: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
Image size: 937.5'x625.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:41:50.925 -34:05:21.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:41:52.558 -34:02:25.57
Second-epoch image center 16:41:50.925 -34:05:21.57
Angular distance between the image centers 0.0492 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits (2nd new image)
verification OK: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
Image size: 937.5'x625.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:41:48.700 -34:04:40.32 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:41:52.558 -34:02:25.57
Second-epoch image center 16:41:48.700 -34:04:40.32
Angular distance between the image centers 0.0397 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 16:41:50.925 -34:05:21.57
Second-epoch second image center 16:41:48.700 -34:04:40.32
Angular distance between the image centers 0.01379 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/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits &> /tmp/tmp.L8Gm9CCg0P
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits &> /tmp/tmp.YeXLxq0b9Z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits &> /tmp/tmp.oOcigvASSq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits &> /tmp/tmp.EFUiq8bFJ0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.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_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits and wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits and wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat
Found non-empty wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits and wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat
The reference image (wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits) and catalog (wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat) found
'wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat' -> 'wcsmag.cat'
Read 79602 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.0348 to 260.1370 deg, Dec -39.5208 to -27.9828 deg
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
Tycho-2 catalog search boundaries: RA 240.0348 to 260.1370 deg, Dec -39.5208 to -27.9828 deg
Loaded 14177 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10230 out of 11267 total matches.
Matched with Tycho-2 11267 out of 79602 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.964800
a=0.000000 b=1.000000 c=21.964800
From vast_summary.log: estimated ref. image limiting mag.: -8.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.93
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.93
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 79602 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.0348 to 260.1370 deg, Dec -39.5208 to -27.9828 deg
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
Tycho-2 catalog search boundaries: RA 240.0348 to 260.1370 deg, Dec -39.5208 to -27.9828 deg
Loaded 14177 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10230 out of 11267 total matches.
Matched with Tycho-2 11267 out of 79602 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits:
Forced-photometry filter: calibrated wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits -> calib.txt_param_ref_wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits (aperture=4.3)
Read 93737 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.4051 to 260.4660 deg, Dec -39.2724 to -28.4700 deg
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
Tycho-2 catalog search boundaries: RA 240.4051 to 260.4660 deg, Dec -39.2724 to -28.4700 deg
Loaded 13415 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 9788 out of 11006 total matches.
Matched with Tycho-2 11006 out of 93737 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits:
Forced-photometry filter: calibrated wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits -> calib.txt_param_ref_wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 73 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
2.1 pix Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
2.0 pix fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
2.0 pix fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
2.0 pix wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
2.1 pix wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
Limiting magnitude estimates:
13.9 mag. Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
14.1 mag. Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
13.8 mag. fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
13.8 mag. fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.L8Gm9CCg0P (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/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits' -> 'wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS-calibrated image found: wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Checking if the catalog wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS catalog name: wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=4102, passed=79585
Got 79585 stars (including 75363 good ones) from the SExtractor catalog wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat
util/solve_plate_with_UCAC5 got 79585 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 312 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 77924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 312 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 77924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 77924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits N_match=961 sigma_overall_arcsec=0.531 sigma_q1_arcsec=0.450 sigma_q2_arcsec=0.488 sigma_q3_arcsec=0.521 sigma_q4_arcsec=0.612 n_q1=218 n_q2=208 n_q3=240 n_q4=295 worst_quadrant_to_overall_ratio=1.153
The image catalog is written to wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits -region wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.YeXLxq0b9Z (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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits' -> 'wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
WCS-calibrated image found: wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
Checking if the catalog wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits
WCS catalog name: wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=5929, passed=93728
Got 93728 stars (including 87659 good ones) from the SExtractor catalog wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat
util/solve_plate_with_UCAC5 got 93728 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...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
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...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 92354 with non-zero local correction accuracy
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...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 92354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 92356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits N_match=960 sigma_overall_arcsec=0.751 sigma_q1_arcsec=0.672 sigma_q2_arcsec=0.968 sigma_q3_arcsec=0.684 sigma_q4_arcsec=0.761 n_q1=188 n_q2=236 n_q3=213 n_q4=323 worst_quadrant_to_overall_ratio=1.289
The image catalog is written to wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits -region wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.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.oOcigvASSq (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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
Checking if the catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
WCS catalog name: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=7, blended=3677, passed=71346
Got 71346 stars (including 67559 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat
util/solve_plate_with_UCAC5 got 71346 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...
Searching UCAC5 zones 253 to 309 (Dec -39.4 to -28.5)
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...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 69605 with non-zero local correction accuracy
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...
Searching UCAC5 zones 253 to 309 (Dec -39.4 to -28.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 69604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 69605 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits N_match=961 sigma_overall_arcsec=0.776 sigma_q1_arcsec=0.663 sigma_q2_arcsec=0.827 sigma_q3_arcsec=0.809 sigma_q4_arcsec=0.769 n_q1=179 n_q2=260 n_q3=199 n_q4=323 worst_quadrant_to_overall_ratio=1.066
The image catalog is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits -region wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.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.EFUiq8bFJ0 (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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
Checking if the catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
WCS catalog name: wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=3704, passed=70798
Got 70798 stars (including 66978 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat
util/solve_plate_with_UCAC5 got 70798 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...
Searching UCAC5 zones 253 to 309 (Dec -39.4 to -28.5)
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...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 69129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.4 to -28.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 69130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 69130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits N_match=962 sigma_overall_arcsec=0.750 sigma_q1_arcsec=0.684 sigma_q2_arcsec=0.813 sigma_q3_arcsec=0.847 sigma_q4_arcsec=0.711 n_q1=188 n_q2=261 n_q3=192 n_q4=321 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits -region wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-24-29_20.00sec_5.00C_LIGHT_0123.fits
Saving fully-calibrated image wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.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_2026-06-04_CI_Sco-03-Q2b1x1_003250_TTUQ2b1x1_3116230_epJPjEYh/wcs_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124.fits
Preparing the HTML report for the field Sco-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:45:12.61 -34:14:19.7: 13.17 +/- 0.10 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:58:00.52 -33:48:58.2: 13.13 +/- 0.10 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:42:45.07 -30:57:21.7: 12.74 +/- 0.07 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:51:18.95 -30:10:52.7: 13.01 +/- 0.09 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:53:12.35 -36:14:15.1: 12.50 +/- 0.06 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:48:59.65 -36:55:46.4: 13.45 +/- 0.14 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:43:40.61 -38:19:19.2: 13.41 +/- 0.17 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:19:50.00 -33:21:47.7: 13.03 +/- 0.09 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:46:26.35 -38:01:25.1: 13.34 +/- 0.14 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:22:26.42 -30:03:35.0: 12.58 +/- 0.06 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:45:12.61 -34:14:19.7: 13.15 +/- 0.08 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:58:00.52 -33:48:58.2: 12.90 +/- 0.08 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:42:45.07 -30:57:21.7: 12.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.06
Forced photometry reference-image weighted average: 13.16 +/- 0.06
Forced photometry reference-image weighted average: 12.73 +/- 0.04
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:51:18.95 -30:10:52.7: 13.23 +/- 0.09 detection
Forced photometry filter REJECTED candidate at 16:45:12.61 -34:14:19.7: ref_mag=13.16 +/- 0.06 new_mean_mag=13.0909 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:58:00.52 -33:48:58.2: ref_mag=12.98 +/- 0.06 new_mean_mag=13.2573 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:42:45.07 -30:57:21.7: ref_mag=12.73 +/- 0.04 new_mean_mag=13.0185 delta=-0.28 (need > 0.90)
Forced photometry reference-image weighted average: 13.12 +/- 0.06
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:43:40.61 -38:19:19.2: 13.48 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 16:51:18.95 -30:10:52.7: ref_mag=13.12 +/- 0.06 new_mean_mag=13.2126 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.45 +/- 0.11
Forced photometry filter REJECTED candidate at 16:43:40.61 -38:19:19.2: ref_mag=13.45 +/- 0.11 new_mean_mag=13.2081 delta=0.24 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:48:59.65 -36:55:46.4: 12.86 +/- 0.07 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:46:26.35 -38:01:25.1: 13.40 +/- 0.12 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:19:50.00 -33:21:47.7: 13.04 +/- 0.08 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:53:12.35 -36:14:15.1: 12.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.06
Forced photometry filter REJECTED candidate at 16:48:59.65 -36:55:46.4: ref_mag=12.98 +/- 0.06 new_mean_mag=13.3454 delta=-0.37 (need > 0.90)
Forced photometry reference-image weighted average: 13.37 +/- 0.09
Forced photometry reference-image weighted average: 13.04 +/- 0.06
Forced photometry filter REJECTED candidate at 16:46:26.35 -38:01:25.1: ref_mag=13.37 +/- 0.09 new_mean_mag=13.2092 delta=0.16 (need > 0.90)
Forced photometry reference-image weighted average: 12.41 +/- 0.04
Forced photometry filter REJECTED candidate at 16:19:50.00 -33:21:47.7: ref_mag=13.04 +/- 0.06 new_mean_mag=13.0992 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:53:12.35 -36:14:15.1: ref_mag=12.41 +/- 0.04 new_mean_mag=13.2580 delta=-0.85 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:22:26.42 -30:03:35.0: 12.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.04
Forced photometry filter REJECTED candidate at 16:22:26.42 -30:03:35.0: ref_mag=12.69 +/- 0.04 new_mean_mag=12.5682 delta=0.12 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:09:51.80 -35:00:34.4: 12.52 +/- 0.07 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:28:44.28 -30:39:56.7: 12.78 +/- 0.07 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:49:24.21 -33:02:50.5: 12.20 +/- 0.04 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:30:18.16 -31:45:57.2: 12.06 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:58:22.79 -30:47:06.4: 12.14 +/- 0.04 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:11:28.36 -35:14:46.9: 11.28 +/- 0.02 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:43:04.42 -32:50:15.2: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:09:51.80 -35:00:34.4: 13.01 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.05
Forced photometry filter REJECTED candidate at 16:09:51.80 -35:00:34.4: ref_mag=12.70 +/- 0.05 new_mean_mag=12.5025 delta=0.20 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:44:27.16 -31:00:33.9: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:30:18.16 -31:45:57.2: 12.10 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:58:22.79 -30:47:06.4: 12.11 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:49:24.21 -33:02:50.5: 12.17 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:28:44.28 -30:39:56.7: 12.70 +/- 0.05 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 17:00:44.36 -36:38:02.0: 14.21 +/- 0.31 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.03
Forced photometry reference-image weighted average: 12.08 +/- 0.02
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Forced photometry reference-image weighted average: 12.73 +/- 0.04
Forced photometry filter REJECTED candidate at 16:58:22.79 -30:47:06.4: ref_mag=12.12 +/- 0.03 new_mean_mag=12.3722 delta=-0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:30:18.16 -31:45:57.2: ref_mag=12.08 +/- 0.02 new_mean_mag=12.2512 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:49:24.21 -33:02:50.5: ref_mag=12.18 +/- 0.02 new_mean_mag=12.5950 delta=-0.41 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:28:44.28 -30:39:56.7: ref_mag=12.73 +/- 0.04 new_mean_mag=12.4248 delta=0.30 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:11:28.36 -35:14:46.9: 11.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.39 +/- 0.01
Forced photometry filter REJECTED candidate at 16:11:28.36 -35:14:46.9: ref_mag=11.39 +/- 0.01 new_mean_mag=11.4657 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:43:04.42 -32:50:15.2: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 17:00:37.84 -37:39:52.7: 13.52 +/- 0.19 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:44:27.16 -31:00:33.9: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 17:00:44.36 -36:38:02.0: 14.12 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.19
Forced photometry filter KEPT candidate at 17:00:44.36 -36:38:02.0: ref_mag=14.16 +/- 0.19 new_mean_mag=12.9244 delta=1.23 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 17:00:37.84 -37:39:52.7: 13.27 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.11
Forced photometry filter REJECTED candidate at 17:00:37.84 -37:39:52.7: ref_mag=13.35 +/- 0.11 new_mean_mag=13.1474 delta=0.20 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:46:45.52 -30:08:29.3: 14.46 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:53:27.94 -36:40:19.6: 13.44 +/- 0.15 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:11:03.63 -32:46:29.1: 12.86 +/- 0.08 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:33:25.51 -30:01:00.6: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:31:08.71 -37:35:13.1: 13.28 +/- 0.13 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:28:35.26 -37:23:06.4: 13.10 +/- 0.11 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:46:45.52 -30:08:29.3: 14.29 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.26
Forced photometry filter KEPT candidate at 16:46:45.52 -30:08:29.3: ref_mag=14.29 +/- 0.26 new_mean_mag=13.0669 delta=1.22 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:53:27.94 -36:40:19.6: 13.55 +/- 0.14 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:33:25.51 -30:01:00.6: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:11:03.63 -32:46:29.1: 12.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.10
Forced photometry filter REJECTED candidate at 16:53:27.94 -36:40:19.6: ref_mag=13.50 +/- 0.10 new_mean_mag=13.2576 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 12.88 +/- 0.05
Forced photometry filter REJECTED candidate at 16:11:03.63 -32:46:29.1: ref_mag=12.88 +/- 0.05 new_mean_mag=12.6614 delta=0.22 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:28:35.26 -37:23:06.4: 12.80 +/- 0.07 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:31:08.71 -37:35:13.1: 13.57 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.06
Forced photometry filter REJECTED candidate at 16:28:35.26 -37:23:06.4: ref_mag=12.89 +/- 0.06 new_mean_mag=12.8342 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.42 +/- 0.09
Forced photometry filter REJECTED candidate at 16:31:08.71 -37:35:13.1: ref_mag=13.42 +/- 0.09 new_mean_mag=13.2120 delta=0.21 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 17:03:01.44 -38:02:48.5: 13.70 +/- 0.21 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 17:03:01.44 -38:02:48.5: 13.83 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.16
Forced photometry filter REJECTED candidate at 17:03:01.44 -38:02:48.5: ref_mag=13.76 +/- 0.16 new_mean_mag=13.4398 delta=0.32 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:46:40.03 -35:30:14.7: 14.59 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:54:27.93 -38:16:13.7: 13.61 +/- 0.19 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:46:40.03 -35:30:14.7: 14.32 +/- 0.24 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:54:27.93 -38:16:13.7: 13.65 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.24
Forced photometry reference-image weighted average: 13.64 +/- 0.12
Forced photometry filter KEPT candidate at 16:46:40.03 -35:30:14.7: ref_mag=14.32 +/- 0.24 new_mean_mag=13.3431 delta=0.98 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:54:27.93 -38:16:13.7: ref_mag=13.64 +/- 0.12 new_mean_mag=13.3120 delta=0.33 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 17:02:21.97 -29:51:44.4: 13.53 +/- 0.17 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 17:01:44.97 -34:49:01.4: 13.50 +/- 0.16 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:55:12.40 -32:07:46.1: 13.69 +/- 0.16 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 17:02:21.97 -29:51:44.4: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.53 +/- 0.17
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 17:01:44.97 -34:49:01.4: 13.78 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 17:02:21.97 -29:51:44.4: ref_mag=13.53 +/- 0.17 new_mean_mag=13.3989 delta=0.13 (need > 0.90)
Forced photometry reference-image weighted average: 13.62 +/- 0.12
Forced photometry filter REJECTED candidate at 17:01:44.97 -34:49:01.4: ref_mag=13.62 +/- 0.12 new_mean_mag=13.6027 delta=0.02 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:55:12.40 -32:07:46.1: 13.57 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.10
Forced photometry filter REJECTED candidate at 16:55:12.40 -32:07:46.1: ref_mag=13.61 +/- 0.10 new_mean_mag=13.4839 delta=0.13 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:56:53.68 -33:51:34.8: 13.83 +/- 0.19 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:56:53.68 -33:51:34.8: 13.91 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.13
Forced photometry filter REJECTED candidate at 16:56:53.68 -33:51:34.8: ref_mag=13.87 +/- 0.13 new_mean_mag=13.4280 delta=0.45 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:25:51.88 -36:43:13.0: 13.30 +/- 0.13 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:54:41.03 -33:15:53.6: 14.50 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 17:03:00.34 -36:33:43.5: 13.54 +/- 0.16 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:25:51.88 -36:43:13.0: 13.50 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.09
Forced photometry filter REJECTED candidate at 16:25:51.88 -36:43:13.0: ref_mag=13.40 +/- 0.09 new_mean_mag=13.1060 delta=0.29 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:54:41.03 -33:15:53.6: 14.70 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 17:03:00.34 -36:33:43.5: 13.58 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.10
Forced photometry filter REJECTED candidate at 17:03:00.34 -36:33:43.5: ref_mag=13.56 +/- 0.10 new_mean_mag=13.4900 delta=0.07 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:58:09.33 -31:53:31.7: 13.67 +/- 0.18 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:56:31.46 -33:18:21.5: 13.55 +/- 0.15 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 17:01:14.46 -31:33:38.8: 13.74 +/- 0.21 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:58:09.33 -31:53:31.7: 13.77 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.12
Forced photometry filter REJECTED candidate at 16:58:09.33 -31:53:31.7: ref_mag=13.72 +/- 0.12 new_mean_mag=13.5219 delta=0.20 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:56:31.46 -33:18:21.5: 13.55 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.10
Forced photometry filter REJECTED candidate at 16:56:31.46 -33:18:21.5: ref_mag=13.55 +/- 0.10 new_mean_mag=13.4224 delta=0.13 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 17:02:19.56 -29:43:09.2: 13.70 +/- 0.19 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 17:01:14.46 -31:33:38.8: 13.84 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.14
Forced photometry filter REJECTED candidate at 17:01:14.46 -31:33:38.8: ref_mag=13.79 +/- 0.14 new_mean_mag=13.5617 delta=0.23 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 17:02:19.56 -29:43:09.2: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.70 +/- 0.19
Forced photometry filter REJECTED candidate at 17:02:19.56 -29:43:09.2: ref_mag=13.70 +/- 0.19 new_mean_mag=13.2941 delta=0.40 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:58:52.52 -29:55:14.6: 13.77 +/- 0.19 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 17:00:09.20 -32:47:22.0: 13.99 +/- 0.24 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:53:55.28 -35:28:59.2: 13.81 +/- 0.19 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:56:41.20 -30:43:03.6: 14.56 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:58:52.52 -29:55:14.6: 13.79 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.12
Forced photometry filter REJECTED candidate at 16:58:52.52 -29:55:14.6: ref_mag=13.78 +/- 0.12 new_mean_mag=13.5136 delta=0.27 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:53:55.28 -35:28:59.2: 13.65 +/- 0.14 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 17:00:09.20 -32:47:22.0: 13.78 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.11
Forced photometry filter REJECTED candidate at 16:53:55.28 -35:28:59.2: ref_mag=13.71 +/- 0.11 new_mean_mag=13.6207 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.85 +/- 0.14
Forced photometry filter REJECTED candidate at 17:00:09.20 -32:47:22.0: ref_mag=13.85 +/- 0.14 new_mean_mag=13.5713 delta=0.28 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:56:41.20 -30:43:03.6: 14.25 +/- 0.22 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:39:55.20 -37:27:59.5: 13.54 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.22
Forced photometry filter REJECTED candidate at 16:56:41.20 -30:43:03.6: ref_mag=14.25 +/- 0.22 new_mean_mag=13.6320 delta=0.61 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:39:55.20 -37:27:59.5: 13.67 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.11
Forced photometry filter REJECTED candidate at 16:39:55.20 -37:27:59.5: ref_mag=13.60 +/- 0.11 new_mean_mag=13.5100 delta=0.09 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:45:01.22 -37:51:02.2: 14.11 +/- 0.28 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:46:45.67 -36:55:38.4: 13.82 +/- 0.21 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:42:27.12 -34:59:25.8: 14.56 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:11:45.14 -30:37:37.3: 14.37 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:39:29.66 -38:18:03.2: 13.62 +/- 0.19 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:45:01.22 -37:51:02.2: 13.66 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.14
Forced photometry filter REJECTED candidate at 16:45:01.22 -37:51:02.2: ref_mag=13.77 +/- 0.14 new_mean_mag=13.6223 delta=0.15 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:46:45.67 -36:55:38.4: 13.76 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.13
Forced photometry filter REJECTED candidate at 16:46:45.67 -36:55:38.4: ref_mag=13.78 +/- 0.13 new_mean_mag=13.6056 delta=0.18 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:11:45.14 -30:37:37.3: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:42:27.12 -34:59:25.8: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:39:29.66 -38:18:03.2: 13.44 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.11
Forced photometry filter REJECTED candidate at 16:39:29.66 -38:18:03.2: ref_mag=13.50 +/- 0.11 new_mean_mag=13.3419 delta=0.16 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:37:11.90 -36:30:36.3: 14.07 +/- 0.23 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:08:26.74 -36:08:09.1: 13.53 +/- 0.18 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:37:11.90 -36:30:36.3: 14.33 +/- 0.26 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:08:26.74 -36:08:09.1: 14.03 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.17
Forced photometry filter REJECTED candidate at 16:37:11.90 -36:30:36.3: ref_mag=14.19 +/- 0.17 new_mean_mag=13.5951 delta=0.59 (need > 0.90)
Forced photometry reference-image weighted average: 13.72 +/- 0.14
Forced photometry filter REJECTED candidate at 16:08:26.74 -36:08:09.1: ref_mag=13.72 +/- 0.14 new_mean_mag=13.1802 delta=0.54 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:16:04.26 -33:30:47.1: 13.19 +/- 0.11 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:42:30.29 -30:13:34.4: 13.97 +/- 0.21 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:46:53.76 -30:12:11.9: 13.61 +/- 0.16 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:16:04.26 -33:30:47.1: 13.47 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.08
Forced photometry filter REJECTED candidate at 16:16:04.26 -33:30:47.1: ref_mag=13.32 +/- 0.08 new_mean_mag=13.2183 delta=0.11 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:42:30.29 -30:13:34.4: 13.85 +/- 0.16 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:46:53.76 -30:12:11.9: 13.51 +/- 0.11 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:30:29.80 -37:25:18.6: 13.86 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.09
Forced photometry reference-image weighted average: 13.89 +/- 0.13
Forced photometry filter REJECTED candidate at 16:42:30.29 -30:13:34.4: ref_mag=13.89 +/- 0.13 new_mean_mag=13.5833 delta=0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:46:53.76 -30:12:11.9: ref_mag=13.54 +/- 0.09 new_mean_mag=13.4530 delta=0.09 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:30:22.69 -37:47:23.7: 13.81 +/- 0.21 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:30:29.80 -37:25:18.6: 14.16 +/- 0.23 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:30:22.69 -37:47:23.7: 13.77 +/- 0.17 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:14:13.23 -33:36:03.0: 13.43 +/- 0.14 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:11:24.19 -34:07:29.8: 14.10 +/- 0.29 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.16
Forced photometry filter REJECTED candidate at 16:30:29.80 -37:25:18.6: ref_mag=13.99 +/- 0.16 new_mean_mag=13.4566 delta=0.54 (need > 0.90)
Forced photometry reference-image weighted average: 13.79 +/- 0.13
Forced photometry filter REJECTED candidate at 16:30:22.69 -37:47:23.7: ref_mag=13.79 +/- 0.13 new_mean_mag=13.4986 delta=0.29 (need > 0.90)
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:14:13.23 -33:36:03.0: 13.68 +/- 0.14 detection
Forced photometry on wcs_Sco-03-Q2b1x1_2026-05-12_01-57-04_20.00sec_-5.00C_LIGHT_0246.fits at 16:11:24.19 -34:07:29.8: 13.98 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.10
Forced photometry reference-image weighted average: 14.02 +/- 0.17
Forced photometry filter REJECTED candidate at 16:14:13.23 -33:36:03.0: ref_mag=13.56 +/- 0.10 new_mean_mag=13.3718 delta=0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:11:24.19 -34:07:29.8: ref_mag=14.02 +/- 0.17 new_mean_mag=13.4250 delta=0.59 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out105973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out105936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106316.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 105791_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105791_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105796_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105796_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105798_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105798_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105800_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105800_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105802_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105802_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105803_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105803_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105811_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105811_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105823_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105823_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105826_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105826_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105827_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105827_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 17:00:10.95 -33:15:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105829_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105829_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105830_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105830_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105834_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105834_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 17:01:19.57 -35:20:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105840_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105840_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105846_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105846_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105850_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105850_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:58:15.58 -30:05:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105851_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105851_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105854_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105854_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105857_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105857_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 105902_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105902_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:56:05.29 -33:30:39.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105919_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105919_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:57:18.69 -33:15:30.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105936_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
Preparing report for the candidate 105936_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
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Considering the candidate 105951_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
Preparing report for the candidate 105951_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
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Considering the candidate 105973_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 105973_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 17:00:44.36 -36:38:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.872 5976695138416218368 255.18546275618 -36.63376559059 12.3561 10.6330 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106020_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106020_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106027_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106027_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:46:45.52 -30:08:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.622 6031021664348134144 251.69018754754 -30.14147742249 13.1486 11.6549 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106030_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106030_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106037_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106037_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106041_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
Preparing report for the candidate 106041_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
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Considering the candidate 106051_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106051_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106073_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106073_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106079_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106079_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106085_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106085_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106089_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106089_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:46:40.03 -35:30:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.245 6020051321439534336 251.66702887829 -35.50379632057 13.0807 11.1738 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106096_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106096_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 17:03:13.05 -34:36:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106102_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106102_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:45:55.67 -30:39:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106112_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106112_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106135_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106135_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106137_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106137_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106138_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106138_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106145_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106145_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:54:41.03 -33:15:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.995 6026678765219472768 253.67142765836 -33.26415516110 12.2252 10.3535 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106156_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106156_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106171_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106171_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106180_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106180_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:57:15.68 -30:41:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106186_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106186_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106189_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106189_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106198_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106198_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106210_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106210_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106211_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106211_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:58:47.79 -30:00:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106216_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106216_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106219_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106219_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106247_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106247_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106273_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106273_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106282_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106282_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106304_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106304_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106307_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106307_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106316_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
Preparing report for the candidate 106316_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
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Considering the candidate 106348_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106348_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106352_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106352_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:42:27.12 -34:59:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.057 6020805277180975744 250.61365737120 -34.98984350682 12.3275 10.9437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106369_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106369_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106372_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106372_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106374_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106374_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106376_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106376_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106379_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106379_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106439_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106439_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106454_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106454_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106466_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106466_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 106526_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 106526_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
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Considering the candidate 91036_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 91036_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:46:01.21 -36:33:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93654_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 93654_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:10:17.16 -30:14:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93194_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 93194_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:11:55.67 -31:05:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92614_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 92614_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks
**** FOUND 16:26:39.39 -31:14:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91433_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124
The candidate 91433_fd_Sco-03-Q2b1x1_2026-06-04_00-25-19_20.00sec_5.00C_LIGHT_0124 did not pass the final checks