This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq
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 09 18.4785 2461301.9785 10.05 07:47:52.25 -27:29:57.1
243.57001 -1.03803 galactic Pup Second-epoch detections are separated by 0.6" and 6.8 pix
The object was found in VSX 0" NSV 3743
Type: M
# Max. Min./Amp. JD0 Period
11.200 V < 14.500 V 2452862.00000 493.000000000000 M8
The object was not found in astcheck.
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:47:52.25 -27:29:57.1: 11.12 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:47:52.25 -27:29:57.1: 11.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.01
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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 3743,2461301.9785,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
NSV 3743 20260918.4785 10.05CV 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 09 18.4785 2461301.9785 12.46 07:35:31.40 -25:42:49.5
240.65157 -2.55312 galactic Pup Second-epoch detections are separated by 1.9" and 6.7 pix
The object was found in VSX 0" GDS_J0735314-254249
Type: VAR
# Max. Min./Amp. JD0 Period
13.520 r Y 0.350 r M8
The object was not found in astcheck.
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:35:31.40 -25:42:49.5: 13.99 +/- 0.12 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:35:31.40 -25:42:49.5: 13.44 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.05
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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0735314-254249,2461301.9785,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
GDS_J0735314-254249 20260918.4785 12.46CV 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 09 18.4785 2461301.9785 12.87 07:40:42.81 -22:10:35.1
238.14756 0.21311 galactic Pup Second-epoch detections are separated by 1.3" and 7.1 pix
The object was found in VSX 1" V0470 Pup
Type: M
# Max. Min./Amp. JD0 Period
11.100 V < 16.700 V 2451959.80000 327.000000000000 M8-M9
The object was not found in astcheck.
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:40:42.81 -22:10:35.1: 13.83 +/- 0.11 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:40:42.81 -22:10:35.1: 13.93 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.07
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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0470 Pup,2461301.9785,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
V0470 Pup 20260918.4785 12.87CV 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 09 18.4785 2461301.9785 11.95 07:35:04.27 -23:59:17.1
239.09178 -1.80544 galactic Pup Second-epoch detections are separated by 2.2" and 6.4 pix
The object was found in VSX 5" DU Pup
Type: M
# Max. Min./Amp. JD0 Period
11.700 V < 15.000 V 2454520.00000 523.000000000000 M7-M10
The object was not found in astcheck.
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:35:04.27 -23:59:17.1: 13.86 +/- 0.10 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:35:04.27 -23:59:17.1: 13.66 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.06
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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DU Pup,2461301.9785,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
DU Pup 20260918.4785 11.95CV 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 09 18.4785 2461301.9785 11.32 07:36:06.18 -30:41:34.5
245.08085 -4.84972 galactic Pup Second-epoch detections are separated by 1.2" and 6.5 pix
The object was found in VSX 1" ASAS J073606-3041.6
Type: MISC
# Max. Min./Amp. JD0 Period
8.809 Ic Y 0.533 Ic 2452871.60000 189.480000000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:36:06.18 -30:41:34.5: 12.28 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:36:06.18 -30:41:34.5: 12.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.02
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
ASAS J073606-3041.6,2461301.9785,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J073606-3041.6 20260918.4785 11.32CV 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: 2461120.58564178 21.03.2026 02:03:09.450 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
First image: 2461120.58564178 21.03.2026 02:03:09.450 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Last image: 2461301.97877752 18.09.2026 11:29:16.378 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.36
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 23526
Objects passed selection criteria: 23473
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 19279.8
Average stars matched: 17278.5 (89.6199 %)
Memory usage VmPeak: 249720 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Sep 18 06:32:21 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: 2461120.58564178 21.03.2026 02:03:09.450 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
First image: 2461120.58564178 21.03.2026 02:03:09.450 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Last image: 2461301.97877752 18.09.2026 11:29:16.378 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 113
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.04
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: 65 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 185965
Objects passed selection criteria: 185579
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 155672
Average stars matched: 142972 (91.8421 %)
Memory usage VmPeak: 587420 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Sep 18 06:34:16 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/TTUQ1b1x1/TTUQ1_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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
SExtractor catalog cache: saved Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.cat to cache
SExtractor catalog cache: saved Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.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/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.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: 2461301.97818250
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits exists and is non-empty
wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits exists and is non-empty
wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits exists and is non-empty
wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits (1st reference image)
verification OK: wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Image size: 937.4'x624.6' 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: 07:40:35.849 -25:59:04.31 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits (1st new image)
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
Image size: 943.8'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:40:36.921 -26:00:49.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:40:35.849 -25:59:04.31
Second-epoch image center 07:40:36.921 -26:00:49.53
Angular distance between the image centers 0.0295 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits (2nd new image)
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
Image size: 943.7'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:40:35.153 -26:00:16.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:40:35.849 -25:59:04.31
Second-epoch image center 07:40:35.153 -26:00:16.56
Angular distance between the image centers 0.0202 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 07:40:36.921 -26:00:49.53
Second-epoch second image center 07:40:35.153 -26:00:16.56
Angular distance between the image centers 0.01130 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits &> /tmp/tmp.7GjQ93QwZf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits &> /tmp/tmp.8yCH0rUCX7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits &> /tmp/tmp.gxg0eXwN7j
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits &> /tmp/tmp.4F61wGbK6w
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
Calibrating the magnitude scale
Found non-empty wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.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_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat
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_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat
Found non-empty wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat
The reference image (wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits) and catalog (wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat) found
'wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat' -> 'wcsmag.cat'
Read 24129 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 106.0664 to 124.2087 deg, Dec -31.2449 to -20.5389 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 106.0664 to 124.2087 deg, Dec -31.2449 to -20.5389 deg
Loaded 32711 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): 17231 out of 18280 total matches.
Matched with Tycho-2 18280 out of 24129 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.803200
a=0.000000 b=1.000000 c=22.803200
From vast_summary.log: estimated ref. image limiting mag.: -8.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.44
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24129 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 106.0664 to 124.2087 deg, Dec -31.2449 to -20.5389 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 106.0664 to 124.2087 deg, Dec -31.2449 to -20.5389 deg
Loaded 32711 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): 17231 out of 18280 total matches.
Matched with Tycho-2 18280 out of 24129 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Forced-photometry filter: calibrated wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits -> calib.txt_param_ref_wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits (aperture=6.4)
Read 31217 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 105.7774 to 123.9815 deg, Dec -31.5188 to -20.0567 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 105.7774 to 123.9815 deg, Dec -31.5188 to -20.0567 deg
Loaded 35019 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): 20687 out of 22203 total matches.
Matched with Tycho-2 22203 out of 31217 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
Forced-photometry filter: calibrated wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits -> calib.txt_param_ref_wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.5 pix Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
2.5 pix Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
2.6 pix fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
2.6 pix fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
Limiting magnitude estimates:
14.4 mag. Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
14.7 mag. Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
13.6 mag. fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
13.6 mag. fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
All-image limiting magnitude estimate: 13.6 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.7GjQ93QwZf (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/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits' -> 'wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Checking if the catalog wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat corresponding to the image wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat corresponding to the image wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
WCS catalog name: wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2196, bad_region=0, passed=24129
Got 24129 stars (including 21914 good ones) from the SExtractor catalog wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat
util/solve_plate_with_UCAC5 got 24129 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.2 to -20.5)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 4821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 24129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.2 to -20.5)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4822 matched stars entering correct_measured_positions(), 24129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 4822 matched stars entering correct_measured_positions(), 24129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 4822 stars left (next iteration limit 5300)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits N_match=4822 sigma_overall_arcsec=0.685 sigma_q1_arcsec=0.498 sigma_q2_arcsec=1.017 sigma_q3_arcsec=0.612 sigma_q4_arcsec=0.795 n_q1=1123 n_q2=1284 n_q3=1145 n_q4=1270 worst_quadrant_to_overall_ratio=1.484
The image catalog is written to wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits -region wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.8yCH0rUCX7 (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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits' -> 'wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
WCS_IMAGE_NAME=wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
WCS-calibrated image found: wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
Checking if the catalog wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits alredy exist and is non-empty...
Catalog wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
WCS catalog name: wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2858, bad_region=0, passed=31217
Got 31217 stars (including 28324 good ones) from the SExtractor catalog wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat
util/solve_plate_with_UCAC5 got 31217 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4804 matched stars entering correct_measured_positions(), 4807 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4804 matched stars entering correct_measured_positions(), 31217 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4804 matched stars entering correct_measured_positions(), 31217 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4804 matched stars entering correct_measured_positions(), 31217 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4804 stars left (next iteration limit 5284)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits N_match=4804 sigma_overall_arcsec=0.516 sigma_q1_arcsec=0.484 sigma_q2_arcsec=0.570 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.572 n_q1=1243 n_q2=1196 n_q3=1286 n_q4=1079 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits -region wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.gxg0eXwN7j (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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
Checking if the catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
WCS catalog name: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=731, bad_region=0, passed=11146
Got 11146 stars (including 10403 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat
util/solve_plate_with_UCAC5 got 11146 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.8'
Seting catalog search parameters based on the expected field of view 943.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013108 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010487 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 4923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4794 matched stars entering correct_measured_positions(), 4797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4793 matched stars entering correct_measured_positions(), 11146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 4923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4794 matched stars entering correct_measured_positions(), 11146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4794 matched stars entering correct_measured_positions(), 11146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 4794 stars left (next iteration limit 5272)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4794 robust_rms=8.064 arcsec worst_quadrant_rms=11.429 arcsec
SIP_REFIT: SIP order 3 trial: matched=4794 robust_rms=0.622 arcsec worst_quadrant_rms=1.110 arcsec
SIP_REFIT: SIP order 5 trial: matched=4794 robust_rms=0.538 arcsec worst_quadrant_rms=0.835 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4794 robust_rms_before=1.192 arcsec robust_rms_before_corrected=0.525 arcsec robust_rms_after=0.538 arcsec worst_quadrant_rms_before=0.792 worst_quadrant_rms_after=0.835
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.792 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits N_match=4794 sigma_overall_arcsec=0.505 sigma_q1_arcsec=0.509 sigma_q2_arcsec=0.750 sigma_q3_arcsec=0.412 sigma_q4_arcsec=0.508 n_q1=1197 n_q2=881 n_q3=1519 n_q4=1197 worst_quadrant_to_overall_ratio=1.486
The image catalog is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits -region wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.4F61wGbK6w (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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
Checking if the catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
WCS catalog name: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=734, bad_region=0, passed=11077
Got 11077 stars (including 10330 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat
util/solve_plate_with_UCAC5 got 11077 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.7'
Seting catalog search parameters based on the expected field of view 943.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013107 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010486 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4795 matched stars entering correct_measured_positions(), 4798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4795 matched stars entering correct_measured_positions(), 11077 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4797 matched stars entering correct_measured_positions(), 11077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4797 matched stars entering correct_measured_positions(), 11077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4797 stars left (next iteration limit 5274)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4797 robust_rms=8.142 arcsec worst_quadrant_rms=11.229 arcsec
SIP_REFIT: SIP order 3 trial: matched=4797 robust_rms=0.586 arcsec worst_quadrant_rms=0.913 arcsec
SIP_REFIT: SIP order 5 trial: matched=4797 robust_rms=0.490 arcsec worst_quadrant_rms=0.784 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4797 robust_rms_before=1.242 arcsec robust_rms_before_corrected=0.527 arcsec robust_rms_after=0.490 arcsec worst_quadrant_rms_before=0.724 worst_quadrant_rms_after=0.784
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.724 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits N_match=4797 sigma_overall_arcsec=0.511 sigma_q1_arcsec=0.521 sigma_q2_arcsec=0.750 sigma_q3_arcsec=0.411 sigma_q4_arcsec=0.501 n_q1=1203 n_q2=888 n_q3=1507 n_q4=1199 worst_quadrant_to_overall_ratio=1.468
The image catalog is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits -region wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits to local_wcs_cache/
'wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits' -> 'local_wcs_cache/wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits'
Saving the final (post-refit) wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits to local_wcs_cache/
'wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits' -> 'local_wcs_cache/wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits'
Saving the final (post-refit) wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits to local_wcs_cache/
'wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits' -> 'local_wcs_cache/wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits'
Saving the final (post-refit) wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits to local_wcs_cache/
'wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits' -> 'local_wcs_cache/wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits sigma_overall=0.685 worst_q_ratio=1.484
ref2=Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits sigma_overall=0.516 worst_q_ratio=1.108
new1=fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits sigma_overall=0.505 worst_q_ratio=1.486
new2=fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits sigma_overall=0.511 worst_q_ratio=1.468
reference average sigma_overall=0.6005 worst_q_ratio=1.296
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013_astrometric_residuals.png (4822 matched stars from wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.70 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000_astrometric_residuals.png (4804 matched stars from wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533_astrometric_residuals.png (4794 matched stars from wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534_astrometric_residuals.png (4797 matched stars from wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits'
Saving fully-calibrated image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits'
Preparing the HTML report for the field Pup-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:47:52.25 -27:29:57.1: 11.12 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:47:52.25 -27:29:57.1: 11.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.01
Forced photometry filter KEPT candidate at 07:47:52.25 -27:29:57.1: ref_mag=11.09 +/- 0.01 new_mean_mag=10.0516 delta=1.04 (need > 0.90)
Adding exclusion_list_local.txt__out08513.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37978_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 37978_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:46:38.26 -26:20:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37991_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 37991_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:24:11.82 -29:16:31.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37992_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 37992_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:18:42.64 -24:55:52.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37996_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 37996_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:13:44.97 -30:34:47.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37999_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 37999_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:24:49.58 -21:28:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08513_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
Preparing report for the candidate 08513_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Pup-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:47:52.25 -27:29:57.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
SExtractor catalog cache: saved Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.cat to cache
SExtractor catalog cache: saved Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Creating symlink local_wcs_cache/wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
Creating symlink local_wcs_cache/wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
Creating symlink local_wcs_cache/wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
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_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits exists and is non-empty
wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits exists and is non-empty
wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits exists and is non-empty
wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits (1st reference image)
verification OK: wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Image size: 937.4'x624.6' 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: 07:40:35.849 -25:59:04.31 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits (1st new image)
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
Image size: 943.8'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:40:36.921 -26:00:49.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:40:35.849 -25:59:04.31
Second-epoch image center 07:40:36.921 -26:00:49.53
Angular distance between the image centers 0.0295 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits (2nd new image)
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
Image size: 943.7'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:40:35.153 -26:00:16.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:40:35.849 -25:59:04.31
Second-epoch image center 07:40:35.153 -26:00:16.56
Angular distance between the image centers 0.0202 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 07:40:36.921 -26:00:49.53
Second-epoch second image center 07:40:35.153 -26:00:16.56
Angular distance between the image centers 0.01130 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits &> /tmp/tmp.EvERstLqy0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits &> /tmp/tmp.BCh0loSJtQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits &> /tmp/tmp.5LqSUXVMDZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits &> /tmp/tmp.jz7qLPSoSd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
Calibrating the magnitude scale
Found non-empty wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.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_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat
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_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat
Found non-empty wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat
The reference image (wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits) and catalog (wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat) found
'wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat' -> 'wcsmag.cat'
Read 195364 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 106.0450 to 124.2402 deg, Dec -31.2531 to -20.5192 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 106.0450 to 124.2402 deg, Dec -31.2531 to -20.5192 deg
Loaded 32868 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): 20340 out of 26729 total matches.
Matched with Tycho-2 26729 out of 195364 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.643400
a=0.000000 b=1.000000 c=22.643400
From vast_summary.log: estimated ref. image limiting mag.: -8.04
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.60
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 195364 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 106.0450 to 124.2402 deg, Dec -31.2531 to -20.5192 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 106.0450 to 124.2402 deg, Dec -31.2531 to -20.5192 deg
Loaded 32868 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): 20340 out of 26729 total matches.
Matched with Tycho-2 26729 out of 195364 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Forced-photometry filter: calibrated wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits -> calib.txt_param_ref_wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits (aperture=4.9)
Read 233070 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 105.7099 to 123.9838 deg, Dec -31.5190 to -20.0298 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 105.7099 to 123.9838 deg, Dec -31.5190 to -20.0298 deg
Loaded 35232 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): 20093 out of 27664 total matches.
Matched with Tycho-2 27664 out of 233070 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
Forced-photometry filter: calibrated wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits -> calib.txt_param_ref_wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 108 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
2.4 pix Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
2.5 pix fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
2.5 pix fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
Limiting magnitude estimates:
14.6 mag. Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
14.8 mag. Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
13.7 mag. fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
13.7 mag. fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.1 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.EvERstLqy0 (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/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits' -> 'wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
Checking if the catalog wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat corresponding to the image wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat corresponding to the image wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits
WCS catalog name: wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=25724, bad_region=1, passed=195305
Got 195305 stars (including 169382 good ones) from the SExtractor catalog wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat
util/solve_plate_with_UCAC5 got 195305 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 4830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 195305 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 195305 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 195305 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 4830 stars left (next iteration limit 5311)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits N_match=4830 sigma_overall_arcsec=0.702 sigma_q1_arcsec=0.521 sigma_q2_arcsec=0.960 sigma_q3_arcsec=0.685 sigma_q4_arcsec=0.795 n_q1=1227 n_q2=1290 n_q3=1106 n_q4=1207 worst_quadrant_to_overall_ratio=1.368
The image catalog is written to wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits -region wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.BCh0loSJtQ (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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits' -> 'wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
WCS_IMAGE_NAME=wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
WCS-calibrated image found: wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
Checking if the catalog wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits alredy exist and is non-empty...
Catalog wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits
WCS catalog name: wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=34569, bad_region=7, passed=233040
Got 233040 stars (including 198161 good ones) from the SExtractor catalog wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat
util/solve_plate_with_UCAC5 got 233040 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 4826 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 233040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 233040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 233040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4825 stars left (next iteration limit 5307)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits N_match=4825 sigma_overall_arcsec=0.506 sigma_q1_arcsec=0.477 sigma_q2_arcsec=0.575 sigma_q3_arcsec=0.420 sigma_q4_arcsec=0.522 n_q1=1187 n_q2=1159 n_q3=1331 n_q4=1148 worst_quadrant_to_overall_ratio=1.135
The image catalog is written to wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits -region wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.5LqSUXVMDZ (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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
Checking if the catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
WCS catalog name: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=6533, bad_region=2, passed=98987
Got 98987 stars (including 92321 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat
util/solve_plate_with_UCAC5 got 98987 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.8'
Seting catalog search parameters based on the expected field of view 943.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013108 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010487 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4810 matched stars entering correct_measured_positions(), 4812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4810 matched stars entering correct_measured_positions(), 98987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 98987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 98987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 4812 stars left (next iteration limit 5291)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4812 robust_rms=8.189 arcsec worst_quadrant_rms=13.665 arcsec
SIP_REFIT: SIP order 3 trial: matched=4812 robust_rms=0.625 arcsec worst_quadrant_rms=1.092 arcsec
SIP_REFIT: SIP order 5 trial: matched=4812 robust_rms=0.541 arcsec worst_quadrant_rms=0.847 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4812 robust_rms_before=1.183 arcsec robust_rms_before_corrected=0.509 arcsec robust_rms_after=0.541 arcsec worst_quadrant_rms_before=0.744 worst_quadrant_rms_after=0.847
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.744 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits N_match=4812 sigma_overall_arcsec=0.496 sigma_q1_arcsec=0.510 sigma_q2_arcsec=0.706 sigma_q3_arcsec=0.407 sigma_q4_arcsec=0.476 n_q1=1239 n_q2=881 n_q3=1516 n_q4=1176 worst_quadrant_to_overall_ratio=1.423
The image catalog is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits -region wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.jz7qLPSoSd (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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
Checking if the catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
WCS catalog name: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=6417, bad_region=2, passed=98356
Got 98356 stars (including 91816 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat
util/solve_plate_with_UCAC5 got 98356 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.7'
Seting catalog search parameters based on the expected field of view 943.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013107 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010486 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4807 matched stars entering correct_measured_positions(), 4810 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4806 matched stars entering correct_measured_positions(), 98356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4806 matched stars entering correct_measured_positions(), 98356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4806 matched stars entering correct_measured_positions(), 98356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4806 stars left (next iteration limit 5286)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4806 robust_rms=8.224 arcsec worst_quadrant_rms=12.838 arcsec
SIP_REFIT: SIP order 3 trial: matched=4806 robust_rms=0.592 arcsec worst_quadrant_rms=0.914 arcsec
SIP_REFIT: SIP order 5 trial: matched=4806 robust_rms=0.490 arcsec worst_quadrant_rms=0.770 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4806 robust_rms_before=1.238 arcsec robust_rms_before_corrected=0.507 arcsec robust_rms_after=0.490 arcsec worst_quadrant_rms_before=0.707 worst_quadrant_rms_after=0.770
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.707 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits N_match=4806 sigma_overall_arcsec=0.495 sigma_q1_arcsec=0.493 sigma_q2_arcsec=0.718 sigma_q3_arcsec=0.412 sigma_q4_arcsec=0.484 n_q1=1254 n_q2=877 n_q3=1486 n_q4=1189 worst_quadrant_to_overall_ratio=1.451
The image catalog is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits -region wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-28-24_20.00sec_-0.00C_LIGHTs_0533.fits
Saving fully-calibrated image wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.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_2026-09-18_CI_Pup-02-Q1b1x1_062949_TTUQ1b1x1_796071_ppoGynEq/wcs_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534.fits
Preparing the HTML report for the field Pup-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:33:50.32 -26:03:16.0: 13.17 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:24:49.36 -28:40:24.5: 12.46 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:32:53.14 -25:38:58.0: 13.10 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:43:37.48 -26:31:52.9: 13.00 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:34:14.56 -26:26:18.8: 13.28 +/- 0.07 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:18:44.15 -24:48:59.5: 12.24 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:45:29.79 -25:49:32.1: 13.02 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:13:05.33 -24:02:40.4: 12.86 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:44:23.63 -31:09:30.6: 12.16 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:24:49.36 -28:40:24.5: 12.52 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:13:05.33 -24:02:40.4: 13.01 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:18:44.15 -24:48:59.5: 12.59 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:34:14.56 -26:26:18.8: 13.32 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:32:53.14 -25:38:58.0: 13.18 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:33:50.32 -26:03:16.0: 13.20 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:43:37.48 -26:31:52.9: 13.09 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:45:29.79 -25:49:32.1: 13.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Forced photometry reference-image weighted average: 12.95 +/- 0.04
Forced photometry filter REJECTED candidate at 07:24:49.36 -28:40:24.5: ref_mag=12.49 +/- 0.02 new_mean_mag=12.5274 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 12.41 +/- 0.02
Forced photometry reference-image weighted average: 13.31 +/- 0.05
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Forced photometry reference-image weighted average: 13.15 +/- 0.04
Forced photometry reference-image weighted average: 13.19 +/- 0.04
Forced photometry filter REJECTED candidate at 07:13:05.33 -24:02:40.4: ref_mag=12.95 +/- 0.04 new_mean_mag=12.9738 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Forced photometry filter REJECTED candidate at 07:18:44.15 -24:48:59.5: ref_mag=12.41 +/- 0.02 new_mean_mag=12.7150 delta=-0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:34:14.56 -26:26:18.8: ref_mag=13.31 +/- 0.05 new_mean_mag=13.2091 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:43:37.48 -26:31:52.9: ref_mag=13.05 +/- 0.03 new_mean_mag=13.1429 delta=-0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:32:53.14 -25:38:58.0: ref_mag=13.15 +/- 0.04 new_mean_mag=13.1774 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:33:50.32 -26:03:16.0: ref_mag=13.19 +/- 0.04 new_mean_mag=13.0857 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:45:29.79 -25:49:32.1: ref_mag=13.02 +/- 0.03 new_mean_mag=13.1046 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:44:23.63 -31:09:30.6: 12.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.02
Forced photometry filter REJECTED candidate at 07:44:23.63 -31:09:30.6: ref_mag=12.17 +/- 0.02 new_mean_mag=12.1918 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:55:08.73 -27:48:56.3: 11.87 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:11:45.89 -23:56:51.6: 12.62 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:11:02.90 -27:55:56.2: 12.28 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:19:53.51 -25:11:01.5: 12.05 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:42:35.50 -23:21:10.9: 12.25 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:20:14.45 -27:08:38.6: 12.60 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:09:59.59 -27:07:23.4: 12.19 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:55:08.73 -27:48:56.3: 11.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter REJECTED candidate at 07:55:08.73 -27:48:56.3: ref_mag=11.90 +/- 0.01 new_mean_mag=12.1698 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:47:27.96 -25:46:54.5: 11.54 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:42:35.50 -23:21:10.9: 12.11 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:20:14.45 -27:08:38.6: 12.68 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:11:45.89 -23:56:51.6: 12.57 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:10:03.78 -27:50:51.5: 11.37 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:19:53.51 -25:11:01.5: 12.05 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:11:02.90 -27:55:56.2: 12.35 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:09:59.59 -27:07:23.4: 12.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Forced photometry reference-image weighted average: 12.59 +/- 0.02
Forced photometry filter REJECTED candidate at 07:20:14.45 -27:08:38.6: ref_mag=12.65 +/- 0.02 new_mean_mag=12.6501 delta=-0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:42:35.50 -23:21:10.9: ref_mag=12.16 +/- 0.02 new_mean_mag=12.1696 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:11:45.89 -23:56:51.6: ref_mag=12.59 +/- 0.02 new_mean_mag=12.7697 delta=-0.18 (need > 0.90)
Forced photometry reference-image weighted average: 12.05 +/- 0.02
Forced photometry reference-image weighted average: 12.32 +/- 0.02
Forced photometry reference-image weighted average: 12.26 +/- 0.02
Forced photometry filter REJECTED candidate at 07:19:53.51 -25:11:01.5: ref_mag=12.05 +/- 0.02 new_mean_mag=12.1223 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:11:02.90 -27:55:56.2: ref_mag=12.32 +/- 0.02 new_mean_mag=12.4880 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:09:59.59 -27:07:23.4: ref_mag=12.26 +/- 0.02 new_mean_mag=12.3219 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:47:27.96 -25:46:54.5: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Forced photometry filter REJECTED candidate at 07:47:27.96 -25:46:54.5: ref_mag=11.53 +/- 0.01 new_mean_mag=11.6600 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:10:03.78 -27:50:51.5: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Forced photometry filter REJECTED candidate at 07:10:03.78 -27:50:51.5: ref_mag=11.41 +/- 0.01 new_mean_mag=11.6741 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 08:08:44.49 -28:50:39.2: 10.92 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:06:29.39 -26:07:32.2: 10.80 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:49:26.68 -26:34:18.2: 11.84 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 08:08:44.49 -28:50:39.2: 10.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.01
Forced photometry filter REJECTED candidate at 08:08:44.49 -28:50:39.2: ref_mag=10.87 +/- 0.01 new_mean_mag=11.0707 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:06:29.39 -26:07:32.2: 11.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.94 +/- 0.01
Forced photometry filter REJECTED candidate at 07:06:29.39 -26:07:32.2: ref_mag=10.94 +/- 0.01 new_mean_mag=11.3918 delta=-0.46 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:53:59.97 -26:18:58.1: 11.57 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:49:26.68 -26:34:18.2: 11.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Forced photometry filter REJECTED candidate at 07:49:26.68 -26:34:18.2: ref_mag=11.73 +/- 0.01 new_mean_mag=11.3094 delta=0.42 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:15:23.47 -28:21:25.1: 12.30 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:53:59.97 -26:18:58.1: 11.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:34:17.41 -25:46:32.1: 12.43 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 07:53:59.97 -26:18:58.1: ref_mag=11.57 +/- 0.01 new_mean_mag=11.6381 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:54:06.64 -26:20:08.5: 12.16 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:24:13.20 -30:09:15.8: 12.62 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:11:49.31 -23:50:24.8: 12.75 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:15:23.47 -28:21:25.1: 12.48 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:44:24.65 -23:51:29.6: 13.12 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.39 +/- 0.02
Forced photometry filter REJECTED candidate at 07:15:23.47 -28:21:25.1: ref_mag=12.39 +/- 0.02 new_mean_mag=12.3880 delta=0.01 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:54:06.64 -26:20:08.5: 12.11 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:50:17.64 -27:59:55.4: 12.32 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:34:17.41 -25:46:32.1: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.02
Forced photometry filter REJECTED candidate at 07:54:06.64 -26:20:08.5: ref_mag=12.13 +/- 0.02 new_mean_mag=12.1513 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Forced photometry filter REJECTED candidate at 07:34:17.41 -25:46:32.1: ref_mag=12.51 +/- 0.02 new_mean_mag=12.4256 delta=0.08 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:24:13.20 -30:09:15.8: 12.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.03
Forced photometry filter REJECTED candidate at 07:24:13.20 -30:09:15.8: ref_mag=12.61 +/- 0.03 new_mean_mag=12.3592 delta=0.25 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:11:49.31 -23:50:24.8: 12.89 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:50:17.64 -27:59:55.4: 12.29 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:44:24.65 -23:51:29.6: 13.33 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.84 +/- 0.03
Forced photometry reference-image weighted average: 12.30 +/- 0.02
Forced photometry filter REJECTED candidate at 07:11:49.31 -23:50:24.8: ref_mag=12.84 +/- 0.03 new_mean_mag=12.8268 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:50:17.64 -27:59:55.4: ref_mag=12.30 +/- 0.02 new_mean_mag=12.3143 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:44:06.46 -24:57:37.8: 12.46 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:32:20.46 -24:02:03.1: 12.82 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:24:53.46 -24:48:26.3: 13.05 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:44:06.46 -24:57:37.8: 12.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.03
Forced photometry filter REJECTED candidate at 07:44:06.46 -24:57:37.8: ref_mag=12.55 +/- 0.03 new_mean_mag=12.5205 delta=0.03 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:32:20.46 -24:02:03.1: 12.83 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:39:55.90 -24:43:32.4: 12.63 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:14:05.15 -21:57:55.5: 13.32 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.03
Forced photometry filter REJECTED candidate at 07:32:20.46 -24:02:03.1: ref_mag=12.82 +/- 0.03 new_mean_mag=12.7250 delta=0.10 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:08:43.02 -23:15:20.1: 14.43 +/- 0.25 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:24:53.46 -24:48:26.3: 12.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Forced photometry filter REJECTED candidate at 07:24:53.46 -24:48:26.3: ref_mag=13.00 +/- 0.03 new_mean_mag=12.9588 delta=0.04 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:39:55.90 -24:43:32.4: 12.74 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:14:05.15 -21:57:55.5: 13.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.03
Forced photometry reference-image weighted average: 13.25 +/- 0.05
Forced photometry filter REJECTED candidate at 07:39:55.90 -24:43:32.4: ref_mag=12.69 +/- 0.03 new_mean_mag=12.6402 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:14:05.15 -21:57:55.5: ref_mag=13.25 +/- 0.05 new_mean_mag=13.2067 delta=0.05 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:08:43.02 -23:15:20.1: 14.43 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.14
Forced photometry filter KEPT candidate at 07:08:43.02 -23:15:20.1: ref_mag=14.43 +/- 0.14 new_mean_mag=13.1496 delta=1.28 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:51:20.70 -29:07:24.9: 14.08 +/- 0.15 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:36:25.70 -27:22:55.9: 15.18 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:18:14.81 -21:10:18.9: 13.15 +/- 0.08 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:07:09.86 -24:46:57.7: 12.97 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:51:20.70 -29:07:24.9: 14.52 +/- 0.20 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:26:45.14 -28:50:01.6: 12.76 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:36:25.70 -27:22:55.9: 15.39 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.24 +/- 0.12
Forced photometry filter KEPT candidate at 07:51:20.70 -29:07:24.9: ref_mag=14.24 +/- 0.12 new_mean_mag=12.5032 delta=1.74 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:18:14.81 -21:10:18.9: 13.20 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:52:23.21 -26:26:51.8: 12.99 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.05
Forced photometry filter REJECTED candidate at 07:18:14.81 -21:10:18.9: ref_mag=13.18 +/- 0.05 new_mean_mag=13.2670 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 08:09:27.58 -23:44:03.6: 14.38 +/- 0.20 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:26:45.14 -28:50:01.6: 12.96 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:07:09.86 -24:46:57.7: 13.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.04
Forced photometry reference-image weighted average: 13.03 +/- 0.04
Forced photometry filter REJECTED candidate at 07:26:45.14 -28:50:01.6: ref_mag=12.87 +/- 0.04 new_mean_mag=12.7512 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:07:09.86 -24:46:57.7: ref_mag=13.03 +/- 0.04 new_mean_mag=13.1486 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:52:23.21 -26:26:51.8: 13.02 +/- 0.11 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:41:16.20 -21:15:07.9: 13.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.08
Forced photometry filter REJECTED candidate at 07:52:23.21 -26:26:51.8: ref_mag=13.01 +/- 0.08 new_mean_mag=12.8180 delta=0.19 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 08:09:27.58 -23:44:03.6: 14.12 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.11
Forced photometry filter KEPT candidate at 08:09:27.58 -23:44:03.6: ref_mag=14.20 +/- 0.11 new_mean_mag=12.8020 delta=1.40 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:41:16.20 -21:15:07.9: 13.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.04
Forced photometry filter REJECTED candidate at 07:41:16.20 -21:15:07.9: ref_mag=13.02 +/- 0.04 new_mean_mag=13.0621 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:22:02.47 -25:51:55.7: 13.03 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:22:02.47 -25:51:55.7: 13.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.04
Forced photometry filter REJECTED candidate at 07:22:02.47 -25:51:55.7: ref_mag=13.07 +/- 0.04 new_mean_mag=13.2203 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:31:54.77 -25:47:31.9: 13.32 +/- 0.07 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:09:46.01 -23:30:34.5: 13.87 +/- 0.15 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:35:14.95 -25:36:44.5: 13.52 +/- 0.08 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:38:44.54 -27:38:21.1: 14.13 +/- 0.15 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:31:54.77 -25:47:31.9: 13.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Forced photometry filter REJECTED candidate at 07:31:54.77 -25:47:31.9: ref_mag=13.34 +/- 0.04 new_mean_mag=13.1999 delta=0.14 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:09:46.01 -23:30:34.5: 13.84 +/- 0.10 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:35:14.95 -25:36:44.5: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.08
Forced photometry filter REJECTED candidate at 07:09:46.01 -23:30:34.5: ref_mag=13.85 +/- 0.08 new_mean_mag=13.6910 delta=0.16 (need > 0.90)
Forced photometry reference-image weighted average: 13.42 +/- 0.05
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:38:44.54 -27:38:21.1: 13.84 +/- 0.09 detection
Forced photometry filter REJECTED candidate at 07:35:14.95 -25:36:44.5: ref_mag=13.42 +/- 0.05 new_mean_mag=13.4608 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 13.92 +/- 0.08
Forced photometry filter REJECTED candidate at 07:38:44.54 -27:38:21.1: ref_mag=13.92 +/- 0.08 new_mean_mag=13.4533 delta=0.46 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:59:16.06 -23:58:50.3: 12.06 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:35:31.40 -25:42:49.5: 13.99 +/- 0.12 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:59:16.06 -23:58:50.3: 11.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 07:59:16.06 -23:58:50.3: ref_mag=12.00 +/- 0.01 new_mean_mag=10.9241 delta=1.08 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 08:14:07.38 -31:00:25.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:40:42.81 -22:10:35.1: 13.83 +/- 0.11 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:35:31.40 -25:42:49.5: 13.44 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.05
Forced photometry filter KEPT candidate at 07:35:31.40 -25:42:49.5: ref_mag=13.55 +/- 0.05 new_mean_mag=12.4577 delta=1.09 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 08:14:07.38 -31:00:25.2: 12.07 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 08:14:07.38 -31:00:25.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:40:42.81 -22:10:35.1: 13.93 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.07
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:35:04.27 -23:59:17.1: 13.86 +/- 0.10 detection
Forced photometry filter KEPT candidate at 07:40:42.81 -22:10:35.1: ref_mag=13.89 +/- 0.07 new_mean_mag=12.8388 delta=1.05 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:58:39.32 -23:12:35.7: 13.35 +/- 0.07 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:36:06.18 -30:41:34.5: 12.28 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:35:04.27 -23:59:17.1: 13.66 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.06
Forced photometry filter KEPT candidate at 07:35:04.27 -23:59:17.1: ref_mag=13.72 +/- 0.06 new_mean_mag=11.9415 delta=1.78 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:58:39.32 -23:12:35.7: 13.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.04
Forced photometry filter REJECTED candidate at 07:58:39.32 -23:12:35.7: ref_mag=13.28 +/- 0.04 new_mean_mag=12.6804 delta=0.60 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:36:06.18 -30:41:34.5: 12.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.02
Forced photometry filter KEPT candidate at 07:36:06.18 -30:41:34.5: ref_mag=12.29 +/- 0.02 new_mean_mag=11.3266 delta=0.97 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out211400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out06886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94144.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 255623_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255623_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255629_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255629_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255635_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255635_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:35:25.90 -24:56:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255649_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255649_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255650_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255650_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255651_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255651_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255678_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255678_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:40:59.05 -23:41:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255680_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255680_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255683_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255683_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255687_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255687_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255690_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255690_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255691_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255691_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:34:40.66 -26:59:31.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255693_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255693_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:22:32.81 -21:23:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255694_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255694_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255697_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255697_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255698_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255698_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255704_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255704_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255705_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255705_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 08:11:26.25 -30:42:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255711_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255711_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255712_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255712_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255715_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255715_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:44:34.06 -23:49:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255716_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255716_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255718_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255718_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255719_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255719_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:25:05.14 -21:01:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255720_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255720_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255723_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255723_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255724_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255724_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255745_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255745_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:44:21.63 -23:53:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255747_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255747_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:13:44.97 -30:34:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255755_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255755_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:24:49.57 -21:28:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255758_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255758_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:44:33.08 -23:50:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255762_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255762_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255764_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255764_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:44:21.97 -23:53:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255770_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255770_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:44:37.00 -23:51:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255771_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255771_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:38:14.69 -25:23:19.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255778_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255778_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255781_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255781_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 08:07:43.73 -24:18:06.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 255792_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255792_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:49:16.91 -24:53:48.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 255793_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255793_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:11:35.27 -20:52:57.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255806_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255806_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:38:23.39 -25:20:54.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255808_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255808_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:16:59.42 -21:11:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255811_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255811_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:24:08.78 -29:20:21.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 255813_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255813_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:59:07.99 -26:49:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255814_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255814_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255816_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255816_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255819_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255819_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255822_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255822_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255826_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255826_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 08:07:11.41 -22:02:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255827_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255827_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:34:41.51 -27:00:34.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255837_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255837_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255838_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255838_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:44:24.65 -23:51:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 0.882 5615568829275538944 116.10254292123 -23.85841508248 12.5960 12.2987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255839_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255839_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255841_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255841_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:14:02.40 -30:20:18.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255844_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255844_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:28:42.99 -29:05:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255846_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255846_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:43:51.72 -28:59:20.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 255850_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255850_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255851_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255851_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:48:19.21 -24:34:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255854_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255854_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255855_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255855_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:37:52.55 -22:36:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255856_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255856_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:11:59.47 -21:45:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255858_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255858_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:48:32.02 -22:41:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255864_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255864_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:13:06.26 -28:30:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255865_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255865_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255866_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255866_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:44:03.79 -24:57:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255869_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255869_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255876_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255876_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:29:45.98 -23:02:30.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255879_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255879_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255881_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255881_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:59:15.34 -22:06:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255882_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255882_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:08:43.02 -23:15:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.913 2927578424842990080 107.17871530333 -23.25538095851 13.2616 11.1415 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255884_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255884_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:29:58.56 -23:00:47.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255885_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255885_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:43:01.89 -22:00:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255887_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255887_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:09:49.93 -22:07:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255889_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255889_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:49:59.90 -23:46:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255890_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255890_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:51:20.70 -29:07:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 1.536 5600326643180259456 117.83576896696 -29.12350904730 11.7155 9.8487 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255893_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255893_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:36:25.70 -27:22:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.649 5612277406859573120 114.10726241811 -27.38210962386 12.6409 10.6142 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255894_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255894_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:22:35.80 -23:08:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255895_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255895_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255896_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255896_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255898_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255898_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255901_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255901_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:38:26.20 -25:21:47.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255902_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255902_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:44:13.88 -23:53:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255907_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255907_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255920_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255920_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 08:09:27.58 -23:44:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.079 5698151670168184064 122.36554157369 -23.73441219165 13.1541 11.3193 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255921_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255921_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255927_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255927_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255937_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255937_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:28:00.57 -22:23:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255938_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255938_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:24:29.40 -27:12:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255944_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255944_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:16:09.01 -23:30:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255954_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255954_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255961_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255961_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 255965_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255965_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255982_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255982_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 255986_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 255986_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 211400_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 211400_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:59:16.06 -23:58:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 2.401 5698657445517651328 119.81683395716 -23.98130155745 10.8453 9.6543 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 94144_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
Preparing report for the candidate 94144_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
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Considering the candidate 177918_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
Preparing report for the candidate 177918_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
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Considering the candidate 79381_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 79381_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:41:05.96 -26:25:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219405_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 219405_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 131366_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
Preparing report for the candidate 131366_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
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Considering the candidate 81511_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 81511_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:46:38.26 -26:20:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06886_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
Preparing report for the candidate 06886_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
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Considering the candidate 209870_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 209870_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
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Considering the candidate 167540_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 167540_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:10:11.07 -21:26:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72782_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 72782_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 08:03:48.59 -26:38:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35162_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 35162_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 08:09:40.03 -28:36:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58759_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 58759_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:47:52.23 -27:29:57.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167433_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 167433_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
**** FOUND 07:24:40.00 -21:33:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72977_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534
The candidate 72977_fd_Pup-02-Q1b1x1_2026-09-18_06-29-16_20.00sec_-0.00C_LIGHTs_0534 did not pass the final checks
