This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6
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 17.4838 2461300.9838 12.71 07:51:04.42 -29:35:35.2
245.73184 -1.49398 galactic Pup Second-epoch detections are separated by 7.3" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:51:04.42 -29:35:35.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:51:04.42 -29:35:35.2: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:51:04.42 -29:35:35.2: 15.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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
target,2461300.9838,12.71,0.05,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
target 20260917.4838 12.71CV 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 17.4838 2461300.9838 11.51 07:41:05.99 -26:25:19.5
241.88305 -1.80771 galactic Pup Second-epoch detections are separated by 0.5" and 9.8 pix
The object was found in VSX 1" V0471 Pup
Type: M
# Max. Min./Amp. JD0 Period
11.000 V < 14.800 V 2454760.00000 380.000000000000 C
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 07:41:05.99 -26:25:19.5: 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 07:41:05.99 -26:25:19.5: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 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
V0471 Pup,2461300.9838,11.51,0.05,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
V0471 Pup 20260917.4838 11.51CV 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 17.4838 2461300.9838 9.23 07:46:38.26 -26:20:36.0
242.43293 -0.69316 galactic Pup Second-epoch detections are separated by 0.2" and 9.8 pix
The object was found in VSX 0" SS Pup
Type: M
# Max. Min./Amp. JD0 Period
12.600 pg 15.700 pg 2426031.00000 391.000000000000 M6e
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 07:46:38.26 -26:20:36.0: 12.33 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:46:38.26 -26:20:36.0: 12.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.33 +/- 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 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
SS Pup,2461300.9838,9.23,0.05,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
SS Pup 20260917.4838 9.23CV 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 17.4838 2461300.9838 12.32 08:03:48.69 -26:38:13.8
244.67274 2.44322 galactic Pup Second-epoch detections are separated by 0.9" and 9.7 pix
The object was found in VSX 1" GDS_J0803486-263813
Type: VAR
# Max. Min./Amp. JD0 Period
13.330 r Y 0.600 r C
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 08:03:48.69 -26:38:13.8: 13.45 +/- 0.09 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 08:03:48.69 -26:38:13.8: 13.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.42 +/- 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_J0803486-263813,2461300.9838,12.32,0.05,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
GDS_J0803486-263813 20260917.4838 12.32CV 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
Mean magnitude and position on the discovery images:
2026 09 17.4838 2461300.9838 11.51 08:09:40.05 -28:36:55.9
247.04032 2.47306 galactic Pup Second-epoch detections are separated by 3.6" and 9.8 pix
The object was found in VSX 3" ASAS J080940-2837.0
Type: M
# Max. Min./Amp. JD0 Period
11.150 V Y 0.440 V 2453156.40000 379.000000000000 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 08:09:40.05 -28:36:55.9: 13.30 +/- 0.08 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 08:09:40.05 -28:36:55.9: 13.48 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.39 +/- 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
ASAS J080940-2837.0,2461300.9838,11.51,0.05,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 J080940-2837.0 20260917.4838 11.51CV 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: 2461300.98421279 17.09.2026 11:37:05.985 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
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: 7 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): 23268
Objects passed selection criteria: 23185
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 16316
Average stars matched: 14309.2 (87.7007 %)
Memory usage VmPeak: 249724 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 Thu Sep 17 06:39:01 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: 2461300.98421279 17.09.2026 11:37:05.985 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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: 191 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): 184332
Objects passed selection criteria: 183892
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 140096
Average stars matched: 127050 (90.6877 %)
Memory usage VmPeak: 652960 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 Thu Sep 17 06:43:36 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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461300.98332972
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits exists and is non-empty
wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits (1st new image)
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
Image size: 943.6'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: 07:40:52.663 -25:59:56.28 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 07:40:52.663 -25:59:56.28
Angular distance between the image centers 0.0646 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits (2nd new image)
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
Image size: 943.5'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: 07:40:55.835 -25:59:15.80 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 07:40:55.835 -25:59:15.80
Angular distance between the image centers 0.0749 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 07:40:52.663 -25:59:56.28
Second-epoch second image center 07:40:55.835 -25:59:15.80
Angular distance between the image centers 0.01636 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.swVZtKjB06
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.2NFMxK3Ybn
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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits &> /tmp/tmp.Dcn4FcjJRT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits &> /tmp/tmp.o6xrPpjx1n
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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 1 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
2.3 pix fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
2.3 pix fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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
13.0 mag. fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
13.0 mag. fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 10.1 (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.swVZtKjB06 (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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/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.2NFMxK3Ybn (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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/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.Dcn4FcjJRT (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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
Checking if the catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
WCS catalog name: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.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=550, bad_region=0, passed=5286
Got 5286 stars (including 4732 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat
util/solve_plate_with_UCAC5 got 5286 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.6'
Seting catalog search parameters based on the expected field of view 943.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013106 (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 0.010484 (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 -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4654 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4529 matched stars entering correct_measured_positions(), 4533 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4528 matched stars entering correct_measured_positions(), 5285 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 -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4654 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4527 matched stars entering correct_measured_positions(), 5285 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4527 matched stars entering correct_measured_positions(), 5285 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4527 stars left (next iteration limit 4980)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4527 robust_rms=8.302 arcsec worst_quadrant_rms=12.010 arcsec
SIP_REFIT: SIP order 3 trial: matched=4527 robust_rms=0.575 arcsec worst_quadrant_rms=0.678 arcsec
SIP_REFIT: SIP order 5 trial: matched=4527 robust_rms=0.482 arcsec worst_quadrant_rms=0.518 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4527 robust_rms_before=1.111 arcsec robust_rms_before_corrected=0.549 arcsec robust_rms_after=0.482 arcsec worst_quadrant_rms_before=0.660 worst_quadrant_rms_after=0.518
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
Image size: 943.8'x627.4' 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: 07:40:52.721 -25:59:57.27 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5286 stars ###
'wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/correct_sextractor_wcs_catalog_usingxy2sky555514.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.111 -> 0.482 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4527 pairs from the initial matching)
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 -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4214 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4214 pairs (4527 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4214 robust_rms=7.762 arcsec worst_quadrant_rms=10.974 arcsec
SIP_REFIT: SIP order 3 trial: matched=4214 robust_rms=0.557 arcsec worst_quadrant_rms=0.630 arcsec
SIP_REFIT: SIP order 5 trial: matched=4214 robust_rms=0.471 arcsec worst_quadrant_rms=0.503 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4214 robust_rms_before=0.472 arcsec robust_rms_before_corrected=0.472 arcsec robust_rms_after=0.471 arcsec worst_quadrant_rms_before=0.503 worst_quadrant_rms_after=0.503
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.503 vs 0.503 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 4214 matched stars entering correct_measured_positions(), 5280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4214 matched stars entering correct_measured_positions(), 5273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WCS_QUALITY_DIAG: file=fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits N_match=4214 sigma_overall_arcsec=0.481 sigma_q1_arcsec=0.434 sigma_q2_arcsec=0.535 sigma_q3_arcsec=0.469 sigma_q4_arcsec=0.500 n_q1=1132 n_q2=695 n_q3=1265 n_q4=1122 worst_quadrant_to_overall_ratio=1.113
The image catalog is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits -region wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.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.o6xrPpjx1n (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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
Checking if the catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
WCS catalog name: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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=645, bad_region=0, passed=5214
Got 5214 stars (including 4565 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat
util/solve_plate_with_UCAC5 got 5214 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.5'
Seting catalog search parameters based on the expected field of view 943.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013104 (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 0.010483 (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 -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4380 matched stars entering correct_measured_positions(), 4385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4379 matched stars entering correct_measured_positions(), 5212 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 -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4377 matched stars entering correct_measured_positions(), 5213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4376 matched stars entering correct_measured_positions(), 5213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 4376 stars left (next iteration limit 4816)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4376 robust_rms=7.917 arcsec worst_quadrant_rms=13.778 arcsec
SIP_REFIT: SIP order 3 trial: matched=4376 robust_rms=0.590 arcsec worst_quadrant_rms=0.869 arcsec
SIP_REFIT: SIP order 5 trial: matched=4376 robust_rms=0.447 arcsec worst_quadrant_rms=0.546 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4376 robust_rms_before=1.123 arcsec robust_rms_before_corrected=0.563 arcsec robust_rms_after=0.447 arcsec worst_quadrant_rms_before=0.811 worst_quadrant_rms_after=0.546
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
Image size: 943.8'x627.4' 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: 07:40:55.892 -25:59:16.76 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5214 stars ###
'wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/correct_sextractor_wcs_catalog_usingxy2sky555519.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.123 -> 0.447 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4376 pairs from the initial matching)
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 -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4063 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4063 pairs (4376 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4063 robust_rms=7.322 arcsec worst_quadrant_rms=11.175 arcsec
SIP_REFIT: SIP order 3 trial: matched=4063 robust_rms=0.562 arcsec worst_quadrant_rms=0.746 arcsec
SIP_REFIT: SIP order 5 trial: matched=4063 robust_rms=0.433 arcsec worst_quadrant_rms=0.502 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4063 robust_rms_before=0.433 arcsec robust_rms_before_corrected=0.433 arcsec robust_rms_after=0.433 arcsec worst_quadrant_rms_before=0.501 worst_quadrant_rms_after=0.502
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.502 vs 0.501 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 4063 matched stars entering correct_measured_positions(), 5210 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4063 matched stars entering correct_measured_positions(), 5209 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
WCS_QUALITY_DIAG: file=fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits N_match=4063 sigma_overall_arcsec=0.446 sigma_q1_arcsec=0.404 sigma_q2_arcsec=0.528 sigma_q3_arcsec=0.456 sigma_q4_arcsec=0.441 n_q1=1064 n_q2=670 n_q3=1303 n_q4=1026 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits -region wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits to local_wcs_cache/
'wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits' -> 'local_wcs_cache/wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits'
Saving the final (post-refit) wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits to local_wcs_cache/
'wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits' -> 'local_wcs_cache/wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits sigma_overall=0.481 worst_q_ratio=1.113
new2=fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits sigma_overall=0.446 worst_q_ratio=1.185
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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123_astrometric_residuals.png (4214 matched stars from wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124_astrometric_residuals.png (4063 matched stars from wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits'
Saving fully-calibrated image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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 07:46:38.27 -26:20:36.0: 12.14 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:46:38.27 -26:20:36.0: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.02
Forced photometry filter KEPT candidate at 07:46:38.27 -26:20:36.0: ref_mag=12.17 +/- 0.02 new_mean_mag=9.1323 delta=3.04 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out37974.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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: 0s
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Considering the candidate 37974_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 37974_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:46:38.27 -26:20:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.13, MAG_FAINT_SEARCH_LIMIT=10.11)GAIADR2_OUTPUT=# 0.283 5601887984053830400 116.65948138057 -26.34325737588 10.0665 8.2905 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
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 ####
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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
Creating symlink local_wcs_cache/wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits exists and is non-empty
wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits (1st new image)
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
Image size: 943.8'x627.4' 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: 07:40:52.721 -25:59:57.27 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 07:40:52.721 -25:59:57.27
Angular distance between the image centers 0.0649 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits (2nd new image)
verification OK: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
Image size: 943.8'x627.4' 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: 07:40:55.892 -25:59:16.76 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 07:40:55.892 -25:59:16.76
Angular distance between the image centers 0.0751 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 07:40:52.721 -25:59:57.27
Second-epoch second image center 07:40:55.892 -25:59:16.76
Angular distance between the image centers 0.01636 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.EY9ddOYkPu
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.mgYlL4DTxt
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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits &> /tmp/tmp.wmAzZetHAE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits &> /tmp/tmp.sZZxm8OKUx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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 105 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
2.1 pix fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
2.1 pix fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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
13.3 mag. fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
13.3 mag. fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 12.7 (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.EY9ddOYkPu (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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/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.mgYlL4DTxt (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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/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.wmAzZetHAE (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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
Checking if the catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
WCS catalog name: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.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=1, no_mag_err=0, low_SNR=44, blended=3492, bad_region=0, passed=67920
Got 67920 stars (including 64341 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat
util/solve_plate_with_UCAC5 got 67920 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 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: 4803 matched stars entering correct_measured_positions(), 4804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 67873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4918 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(), 67873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 67873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4803 stars left (next iteration limit 5283)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.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=4803 robust_rms=7.574 arcsec worst_quadrant_rms=12.350 arcsec
SIP_REFIT: SIP order 3 trial: matched=4803 robust_rms=0.553 arcsec worst_quadrant_rms=0.639 arcsec
SIP_REFIT: SIP order 5 trial: matched=4803 robust_rms=0.469 arcsec worst_quadrant_rms=0.504 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4803 robust_rms_before=0.470 arcsec robust_rms_before_corrected=0.473 arcsec robust_rms_after=0.469 arcsec worst_quadrant_rms_before=0.507 worst_quadrant_rms_after=0.504
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.507 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits N_match=4803 sigma_overall_arcsec=0.471 sigma_q1_arcsec=0.434 sigma_q2_arcsec=0.549 sigma_q3_arcsec=0.466 sigma_q4_arcsec=0.443 n_q1=1394 n_q2=810 n_q3=1370 n_q4=1229 worst_quadrant_to_overall_ratio=1.165
The image catalog is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits -region wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.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.sZZxm8OKUx (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_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
WCS_IMAGE_NAME=wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
WCS-calibrated image found: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
Checking if the catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat corresponding to the image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
WCS catalog name: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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=1, no_mag_err=0, low_SNR=82, blended=3604, bad_region=0, passed=67052
Got 67052 stars (including 63355 good ones) from the SExtractor catalog wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat
util/solve_plate_with_UCAC5 got 67052 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 -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 4811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 67033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4926 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(), 67034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 67034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 4812 stars left (next iteration limit 5292)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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=7.290 arcsec worst_quadrant_rms=12.439 arcsec
SIP_REFIT: SIP order 3 trial: matched=4812 robust_rms=0.554 arcsec worst_quadrant_rms=0.757 arcsec
SIP_REFIT: SIP order 5 trial: matched=4812 robust_rms=0.431 arcsec worst_quadrant_rms=0.496 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4812 robust_rms_before=0.433 arcsec robust_rms_before_corrected=0.458 arcsec robust_rms_after=0.431 arcsec worst_quadrant_rms_before=0.490 worst_quadrant_rms_after=0.496
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.490 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits N_match=4812 sigma_overall_arcsec=0.466 sigma_q1_arcsec=0.429 sigma_q2_arcsec=0.568 sigma_q3_arcsec=0.459 sigma_q4_arcsec=0.423 n_q1=1336 n_q2=829 n_q3=1443 n_q4=1204 worst_quadrant_to_overall_ratio=1.220
The image catalog is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits -region wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-35-49_20.00sec_-0.00C_LIGHTs_0123.fits
Saving fully-calibrated image wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Pup-02-Q1b1x1_063749_TTUQ1b1x1_546785_CThXgsj6/wcs_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124.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 07:39:45.95 -27:18:20.2: 12.96 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:33:40.45 -26:04:29.6: 12.80 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:37:40.74 -26:27:19.0: 12.47 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:26:06.21 -26:56:54.2: 13.03 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:35:06.00 -24:48:16.7: 12.71 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:46:13.00 -26:01:22.5: 12.32 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:40:27.72 -26:04:19.8: 12.63 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:45:43.40 -24:51:01.4: 12.54 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:38:39.96 -25:51:52.1: 12.95 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:30:29.71 -24:07:53.7: 12.72 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:39:45.95 -27:18:20.2: 12.92 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:46:13.00 -26:01:22.5: 12.37 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:38:39.96 -25:51:52.1: 12.96 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:30:29.71 -24:07:53.7: 12.70 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:33:40.45 -26:04:29.6: 12.74 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:26:06.21 -26:56:54.2: 13.08 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:37:40.74 -26:27:19.0: 12.49 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:40:27.72 -26:04:19.8: 12.67 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:45:43.40 -24:51:01.4: 12.54 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:35:06.00 -24:48:16.7: 12.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.03
Forced photometry reference-image weighted average: 12.96 +/- 0.03
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Forced photometry reference-image weighted average: 12.76 +/- 0.03
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry reference-image weighted average: 12.71 +/- 0.03
Forced photometry reference-image weighted average: 13.06 +/- 0.04
Forced photometry reference-image weighted average: 12.54 +/- 0.02
Forced photometry reference-image weighted average: 12.73 +/- 0.03
Forced photometry filter REJECTED candidate at 07:39:45.95 -27:18:20.2: ref_mag=12.93 +/- 0.03 new_mean_mag=12.8572 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:38:39.96 -25:51:52.1: ref_mag=12.96 +/- 0.03 new_mean_mag=12.9796 delta=-0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:46:13.00 -26:01:22.5: ref_mag=12.35 +/- 0.02 new_mean_mag=12.5227 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:33:40.45 -26:04:29.6: ref_mag=12.76 +/- 0.03 new_mean_mag=12.8283 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:37:40.74 -26:27:19.0: ref_mag=12.48 +/- 0.02 new_mean_mag=12.6622 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:40:27.72 -26:04:19.8: ref_mag=12.65 +/- 0.02 new_mean_mag=12.6997 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:30:29.71 -24:07:53.7: ref_mag=12.71 +/- 0.03 new_mean_mag=13.0062 delta=-0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:26:06.21 -26:56:54.2: ref_mag=13.06 +/- 0.04 new_mean_mag=13.1815 delta=-0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:45:43.40 -24:51:01.4: ref_mag=12.54 +/- 0.02 new_mean_mag=12.6959 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:35:06.00 -24:48:16.7: ref_mag=12.73 +/- 0.03 new_mean_mag=12.8170 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 07:59:21.36 -24:14:20.2: 12.13 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:34:50.68 -27:13:30.6: 12.49 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:23:02.39 -25:53:56.7: 12.38 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:38:15.24 -21:29:00.1: 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 07:40:06.57 -24:27:09.3: 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 07:11:03.04 -27:55:57.2: 12.14 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:41:22.05 -27:56:44.1: 12.34 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:28:23.70 -22:45:37.7: 12.33 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:39:08.60 -27:45:47.3: 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 07:59:21.36 -24:14:20.2: 12.10 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:33:01.45 -28:53:05.4: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.02
Forced photometry filter REJECTED candidate at 07:59:21.36 -24:14:20.2: ref_mag=12.11 +/- 0.02 new_mean_mag=12.2803 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:11:03.04 -27:55:57.2: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.02
Forced photometry filter REJECTED candidate at 07:11:03.04 -27:55:57.2: ref_mag=12.19 +/- 0.02 new_mean_mag=12.4765 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:23:02.39 -25:53:56.7: 12.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Forced photometry filter REJECTED candidate at 07:23:02.39 -25:53:56.7: ref_mag=12.45 +/- 0.02 new_mean_mag=12.6194 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:38:15.24 -21:29:00.1: 12.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:34:50.68 -27:13:30.6: 12.60 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 07:38:15.24 -21:29:00.1: ref_mag=12.56 +/- 0.02 new_mean_mag=12.5770 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:40:06.57 -24:27:09.3: 12.35 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:28:23.70 -22:45:37.7: 12.22 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:39:08.60 -27:45:47.3: 12.33 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:41:22.05 -27:56:44.1: 12.32 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 07:34:50.68 -27:13:30.6: ref_mag=12.55 +/- 0.02 new_mean_mag=12.4831 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 12.30 +/- 0.02
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry reference-image weighted average: 12.31 +/- 0.02
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry filter REJECTED candidate at 07:28:23.70 -22:45:37.7: ref_mag=12.25 +/- 0.02 new_mean_mag=12.7232 delta=-0.47 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:40:06.57 -24:27:09.3: ref_mag=12.30 +/- 0.02 new_mean_mag=12.4586 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:39:08.60 -27:45:47.3: ref_mag=12.31 +/- 0.02 new_mean_mag=12.4386 delta=-0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:41:22.05 -27:56:44.1: ref_mag=12.33 +/- 0.02 new_mean_mag=12.4577 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 07:33:01.45 -28:53:05.4: 12.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.02
Forced photometry filter REJECTED candidate at 07:33:01.45 -28:53:05.4: ref_mag=12.15 +/- 0.02 new_mean_mag=12.3787 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:16:16.18 -28:03:25.7: 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 07:18:48.93 -28:36:37.4: 12.66 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:46:48.68 -25:56:33.4: 12.00 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:44:16.06 -23:48:56.6: 12.18 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:45:41.59 -24:47:07.8: 12.09 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:37:50.99 -26:32:45.0: 11.94 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:49:27.02 -26:20:04.1: 11.77 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:56:33.80 -27:16:59.5: 11.89 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:27:41.13 -26:45:18.8: 12.18 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:18:48.93 -28:36:37.4: 12.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.03
Forced photometry filter REJECTED candidate at 07:18:48.93 -28:36:37.4: ref_mag=12.68 +/- 0.03 new_mean_mag=12.5523 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 07:16:16.18 -28:03:25.7: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Forced photometry filter REJECTED candidate at 07:16:16.18 -28:03:25.7: ref_mag=12.38 +/- 0.02 new_mean_mag=12.5191 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 07:46:48.68 -25:56:33.4: 11.98 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 08:00:18.81 -27:56:35.8: 12.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter REJECTED candidate at 07:46:48.68 -25:56:33.4: ref_mag=11.99 +/- 0.01 new_mean_mag=12.3865 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:44:16.06 -23:48:56.6: 12.24 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:45:41.59 -24:47:07.8: 12.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.02
Forced photometry filter REJECTED candidate at 07:44:16.06 -23:48:56.6: ref_mag=12.22 +/- 0.02 new_mean_mag=12.3696 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter REJECTED candidate at 07:45:41.59 -24:47:07.8: ref_mag=12.09 +/- 0.01 new_mean_mag=12.3250 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:56:33.80 -27:16:59.5: 11.87 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:37:50.99 -26:32:45.0: 11.96 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:49:27.02 -26:20:04.1: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Forced photometry filter REJECTED candidate at 07:56:33.80 -27:16:59.5: ref_mag=11.88 +/- 0.01 new_mean_mag=12.0333 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:27:41.13 -26:45:18.8: 12.18 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 07:37:50.99 -26:32:45.0: ref_mag=11.95 +/- 0.01 new_mean_mag=12.3128 delta=-0.36 (need > 0.90)
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Forced photometry filter REJECTED candidate at 07:49:27.02 -26:20:04.1: ref_mag=11.68 +/- 0.01 new_mean_mag=12.0663 delta=-0.39 (need > 0.90)
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter REJECTED candidate at 07:27:41.13 -26:45:18.8: ref_mag=12.18 +/- 0.01 new_mean_mag=12.4160 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 08:00:18.81 -27:56:35.8: 11.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.02
Forced photometry filter REJECTED candidate at 08:00:18.81 -27:56:35.8: ref_mag=11.90 +/- 0.02 new_mean_mag=12.0271 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:10:36.16 -29:51:09.4: 12.08 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:51:33.10 -24:51:51.2: 11.86 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:45:44.99 -28:06:48.9: 11.71 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 08:05:06.93 -28:10:20.1: 11.51 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:44:28.73 -26:44:23.6: 11.86 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:56:33.15 -23:38:03.4: 11.75 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:15:39.59 -27:47:02.6: 11.85 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:10:36.16 -29:51:09.4: 12.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.02
Forced photometry filter REJECTED candidate at 07:10:36.16 -29:51:09.4: ref_mag=12.22 +/- 0.02 new_mean_mag=12.3840 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:51:33.10 -24:51:51.2: 11.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Forced photometry filter REJECTED candidate at 07:51:33.10 -24:51:51.2: ref_mag=11.84 +/- 0.01 new_mean_mag=11.8665 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:45:44.99 -28:06:48.9: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Forced photometry filter REJECTED candidate at 07:45:44.99 -28:06:48.9: ref_mag=11.68 +/- 0.01 new_mean_mag=12.0371 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:25:42.13 -27:54:07.0: 11.92 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 08:05:06.93 -28:10:20.1: 11.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.01
Forced photometry filter REJECTED candidate at 08:05:06.93 -28:10:20.1: ref_mag=11.47 +/- 0.01 new_mean_mag=12.0050 delta=-0.53 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:10:17.59 -29:27:00.3: 11.58 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:44:28.73 -26:44:23.6: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter REJECTED candidate at 07:44:28.73 -26:44:23.6: ref_mag=11.77 +/- 0.01 new_mean_mag=11.9647 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 07:56:33.15 -23:38:03.4: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Forced photometry filter REJECTED candidate at 07:56:33.15 -23:38:03.4: ref_mag=11.71 +/- 0.01 new_mean_mag=11.9782 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:15:39.59 -27:47:02.6: 11.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter REJECTED candidate at 07:15:39.59 -27:47:02.6: ref_mag=11.90 +/- 0.01 new_mean_mag=12.1427 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:25:42.13 -27:54:07.0: 11.91 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:15:08.25 -27:54:59.0: 13.72 +/- 0.13 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Forced photometry filter REJECTED candidate at 07:25:42.13 -27:54:07.0: ref_mag=11.91 +/- 0.01 new_mean_mag=12.0939 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:10:17.59 -29:27:00.3: 11.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Forced photometry filter REJECTED candidate at 07:10:17.59 -29:27:00.3: ref_mag=11.67 +/- 0.01 new_mean_mag=12.0180 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:49:15.22 -25:45:48.3: 11.26 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:47:28.47 -25:47:10.2: 11.61 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:40:11.66 -28:32:22.1: 11.63 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:15:08.25 -27:54:59.0: 13.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.06
Forced photometry filter KEPT candidate at 07:15:08.25 -27:54:59.0: ref_mag=13.43 +/- 0.06 new_mean_mag=11.9852 delta=1.44 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:10:03.83 -27:50:51.0: 11.35 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:49:15.22 -25:45:48.3: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Forced photometry filter REJECTED candidate at 07:49:15.22 -25:45:48.3: ref_mag=11.27 +/- 0.01 new_mean_mag=11.4622 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 07:47:28.47 -25:47:10.2: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.01
Forced photometry filter REJECTED candidate at 07:47:28.47 -25:47:10.2: ref_mag=11.61 +/- 0.01 new_mean_mag=11.6463 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 07:47:18.48 -23:17:00.9: 11.10 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:44:34.02 -23:51:11.4: 9.75 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:40:11.66 -28:32:22.1: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.01
Forced photometry filter REJECTED candidate at 07:40:11.66 -28:32:22.1: ref_mag=11.61 +/- 0.01 new_mean_mag=11.6268 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:10:03.83 -27:50:51.0: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.01
Forced photometry filter REJECTED candidate at 07:10:03.83 -27:50:51.0: ref_mag=11.38 +/- 0.01 new_mean_mag=11.5847 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:52:55.50 -25:42:12.8: 10.82 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:18:01.66 -28:43:49.3: 11.44 +/- 0.01 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:47:18.48 -23:17:00.9: 11.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.01
Forced photometry filter REJECTED candidate at 07:47:18.48 -23:17:00.9: ref_mag=11.12 +/- 0.01 new_mean_mag=11.3703 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 07:44:34.02 -23:51:11.4: 9.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.01
Forced photometry filter REJECTED candidate at 07:44:34.02 -23:51:11.4: ref_mag=9.75 +/- 0.01 new_mean_mag=9.8400 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 07:52:55.50 -25:42:12.8: 10.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.77 +/- 0.01
Forced photometry filter REJECTED candidate at 07:52:55.50 -25:42:12.8: ref_mag=10.77 +/- 0.01 new_mean_mag=10.8527 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 07:18:01.66 -28:43:49.3: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.01
Forced photometry filter REJECTED candidate at 07:18:01.66 -28:43:49.3: ref_mag=11.50 +/- 0.01 new_mean_mag=11.4629 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 07:49:27.06 -26:34:21.2: 11.78 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:54:00.00 -26:18:57.5: 11.58 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:34:07.60 -28:48:56.0: 12.43 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:30:05.43 -25:08:03.5: 12.31 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:24:38.15 -26:41:48.4: 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 07:49:27.06 -26:34:21.2: 11.62 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:54:00.00 -26:18:57.5: 11.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Forced photometry filter REJECTED candidate at 07:49:27.06 -26:34:21.2: ref_mag=11.68 +/- 0.01 new_mean_mag=11.6104 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 11.58 +/- 0.01
Forced photometry filter REJECTED candidate at 07:54:00.00 -26:18:57.5: ref_mag=11.58 +/- 0.01 new_mean_mag=11.6110 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:23:48.47 -23:47:36.8: 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 07:38:15.97 -26:52:46.8: 12.42 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:34:07.60 -28:48:56.0: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Forced photometry filter REJECTED candidate at 07:34:07.60 -28:48:56.0: ref_mag=12.28 +/- 0.02 new_mean_mag=12.1600 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 07:30:05.43 -25:08:03.5: 12.31 +/- 0.02 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:15:23.50 -28:21:25.5: 12.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.02
Forced photometry filter REJECTED candidate at 07:30:05.43 -25:08:03.5: ref_mag=12.31 +/- 0.02 new_mean_mag=12.2204 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 07:24:38.15 -26:41:48.4: 12.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Forced photometry filter REJECTED candidate at 07:24:38.15 -26:41:48.4: ref_mag=12.35 +/- 0.02 new_mean_mag=12.2640 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 07:23:48.47 -23:47:36.8: 12.69 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:38:15.97 -26:52:46.8: 12.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Forced photometry filter REJECTED candidate at 07:23:48.47 -23:47:36.8: ref_mag=12.67 +/- 0.02 new_mean_mag=12.4833 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Forced photometry filter REJECTED candidate at 07:38:15.97 -26:52:46.8: ref_mag=12.45 +/- 0.02 new_mean_mag=12.3183 delta=0.13 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:25:32.16 -24:41:07.2: 12.72 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:15:23.50 -28:21:25.5: 12.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.02
Forced photometry filter REJECTED candidate at 07:15:23.50 -28:21:25.5: ref_mag=12.40 +/- 0.02 new_mean_mag=12.4597 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:23:36.75 -22:57:08.6: 12.74 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:44:06.55 -24:57:35.7: 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 07:34:17.32 -25:46:32.1: 12.42 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:25:32.16 -24:41:07.2: 12.91 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:47:37.55 -27:11:21.4: 12.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.03
Forced photometry filter REJECTED candidate at 07:25:32.16 -24:41:07.2: ref_mag=12.83 +/- 0.03 new_mean_mag=12.6688 delta=0.16 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:39:59.28 -23:21:17.5: 12.72 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:40:07.05 -24:31:24.9: 12.53 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:28:10.20 -29:36:46.9: 12.52 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:23:36.75 -22:57:08.6: 12.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.03
Forced photometry filter REJECTED candidate at 07:23:36.75 -22:57:08.6: ref_mag=12.71 +/- 0.03 new_mean_mag=12.8020 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 07:44:06.55 -24:57:35.7: 12.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.03
Forced photometry filter REJECTED candidate at 07:44:06.55 -24:57:35.7: ref_mag=12.53 +/- 0.03 new_mean_mag=12.4334 delta=0.10 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:34:17.32 -25:46:32.1: 12.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Forced photometry filter REJECTED candidate at 07:34:17.32 -25:46:32.1: ref_mag=12.50 +/- 0.02 new_mean_mag=12.5521 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 07:47:37.55 -27:11:21.4: 12.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.02
Forced photometry filter REJECTED candidate at 07:47:37.55 -27:11:21.4: ref_mag=12.29 +/- 0.02 new_mean_mag=12.4388 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 07:37:52.60 -22:36:58.3: 12.67 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:39:59.28 -23:21:17.5: 12.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.03
Forced photometry filter REJECTED candidate at 07:39:59.28 -23:21:17.5: ref_mag=12.74 +/- 0.03 new_mean_mag=12.7017 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 07:59:08.00 -26:49:43.1: 15.08 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:40:07.05 -24:31:24.9: 12.61 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:28:10.20 -29:36:46.9: 12.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.03
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Forced photometry filter REJECTED candidate at 07:40:07.05 -24:31:24.9: ref_mag=12.58 +/- 0.03 new_mean_mag=12.5770 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:28:10.20 -29:36:46.9: ref_mag=12.49 +/- 0.02 new_mean_mag=12.6210 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:32:20.36 -24:02:03.2: 12.84 +/- 0.05 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:37:52.60 -22:36:58.3: 12.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.03
Forced photometry filter REJECTED candidate at 07:37:52.60 -22:36:58.3: ref_mag=12.66 +/- 0.03 new_mean_mag=12.8211 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:59:08.00 -26:49:43.1: 15.28 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 08:02:20.60 -26:04:24.7: 12.55 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:48:37.08 -27:00:34.3: 12.95 +/- 0.06 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:32:20.36 -24:02:03.2: 12.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.03
Forced photometry filter REJECTED candidate at 07:32:20.36 -24:02:03.2: ref_mag=12.84 +/- 0.03 new_mean_mag=12.7780 delta=0.06 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:51:04.42 -29:35:35.2: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:37:46.32 -26:23:55.9: 12.59 +/- 0.04 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 08:02:20.60 -26:04:24.7: 12.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Forced photometry filter REJECTED candidate at 08:02:20.60 -26:04:24.7: ref_mag=12.56 +/- 0.02 new_mean_mag=12.4967 delta=0.06 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:59:16.07 -23:58:50.3: 12.06 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:48:37.08 -27:00:34.3: 12.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.04
Forced photometry filter REJECTED candidate at 07:48:37.08 -27:00:34.3: ref_mag=12.97 +/- 0.04 new_mean_mag=12.8268 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 07:51:04.42 -29:35:35.2: 15.24 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:37:46.32 -26:23:55.9: 12.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.03
Forced photometry filter REJECTED candidate at 07:37:46.32 -26:23:55.9: ref_mag=12.68 +/- 0.03 new_mean_mag=12.9614 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:59:16.07 -23:58:50.3: 11.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter REJECTED candidate at 07:59:16.07 -23:58:50.3: ref_mag=12.00 +/- 0.01 new_mean_mag=11.1129 delta=0.89 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:41:05.99 -26:25:19.5: 12.52 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 07:46:38.26 -26:20:36.0: 12.33 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 08:03:48.69 -26:38:13.8: 13.45 +/- 0.09 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 07:41:05.99 -26:25:19.5: 12.64 +/- 0.03 detection
Forced photometry on wcs_Pup-02-Q1b1x1_2026-03-20_21-03-09_20.00sec_-15.00C_LIGHT_0013.fits at 08:09:40.05 -28:36:55.9: 13.30 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.02
Forced photometry filter KEPT candidate at 07:41:05.99 -26:25:19.5: ref_mag=12.59 +/- 0.02 new_mean_mag=11.4959 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 07:46:38.26 -26:20:36.0: 12.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry filter KEPT candidate at 07:46:38.26 -26:20:36.0: ref_mag=12.33 +/- 0.02 new_mean_mag=9.2295 delta=3.10 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 08:03:48.69 -26:38:13.8: 13.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.05
Forced photometry filter KEPT candidate at 08:03:48.69 -26:38:13.8: ref_mag=13.42 +/- 0.05 new_mean_mag=12.3054 delta=1.11 (need > 0.90)
Forced photometry on wcs_Pup-02-Q1b1x1_2026-04-05_21-28-35_20.00sec_-4.90C_LIGHTs_0000.fits at 08:09:40.05 -28:36:55.9: 13.48 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.06
Forced photometry filter KEPT candidate at 08:09:40.05 -28:36:55.9: ref_mag=13.39 +/- 0.06 new_mean_mag=11.5099 delta=1.88 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out255759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out256365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81511.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 27s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 255628_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255628_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255633_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255633_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255639_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255639_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255645_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255645_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255654_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255654_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255664_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255664_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255669_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255669_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255674_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255674_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255676_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255676_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255683_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255683_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255685_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255685_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255687_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255687_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255694_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255694_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:40:59.05 -23:41:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255696_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255696_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255697_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255697_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255701_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255701_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255703_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255703_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255704_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255704_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255711_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255711_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255712_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255712_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255716_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255716_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255717_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255717_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255718_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255718_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255719_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255719_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255720_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255720_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255722_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255722_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255724_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255724_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255725_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255725_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255726_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255726_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255731_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255731_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255734_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255734_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255736_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255736_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255737_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255737_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255739_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255739_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255742_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255742_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255746_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255746_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255747_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255747_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255749_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255749_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 08:13:06.93 -24:24:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255750_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255750_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255753_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255753_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:54:37.25 -22:57:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255754_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255754_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255757_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255757_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255758_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255758_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:44:34.11 -23:49:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255759_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255759_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:15:08.25 -27:54:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.824 5609847142561239680 108.78386243542 -27.91661618289 12.3602 10.4164 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255760_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255760_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255761_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255761_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:10:03.53 -30:26:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255762_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255762_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255763_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255763_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255765_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255765_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:41:15.57 -22:19:51.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255767_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255767_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:36:45.99 -30:58:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255769_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255769_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255770_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255770_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 08:04:10.08 -27:28:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255771_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255771_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255781_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255781_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255782_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255782_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:44:33.64 -23:51:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255792_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255792_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:44:21.63 -23:53:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255794_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255794_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255797_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255797_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:13:44.98 -30:34:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255804_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255804_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255805_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255805_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:44:33.13 -23:50:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255810_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255810_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:44:21.98 -23:53:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255822_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255822_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:44:37.15 -23:51:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255824_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255824_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:38:14.75 -25:23:18.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255826_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255826_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:08:10.42 -26:23:57.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 255827_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255827_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255829_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255829_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255840_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255840_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:49:22.73 -24:49:49.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 255845_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255845_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:49:16.97 -24:53:49.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 255849_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255849_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:11:35.15 -20:52:56.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255857_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255857_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:23:50.73 -30:13:03.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255879_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255879_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255884_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255884_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255894_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255894_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255905_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255905_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:38:23.34 -25:20:54.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255907_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255907_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 08:07:43.80 -24:18:08.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 255912_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255912_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255946_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255946_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255964_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255964_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255978_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255978_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:48:19.30 -24:34:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255988_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255988_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 255992_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 255992_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:34:41.55 -27:00:34.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256002_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256002_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 256012_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256012_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256014_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256014_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256052_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256052_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256059_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256059_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256060_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256060_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256072_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256072_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256168_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256168_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256171_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256171_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256178_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256178_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:59:08.00 -26:49:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.333 5601251190713939712 119.78300501376 -26.82841228913 13.1363 10.9936 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256223_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256223_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256225_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256225_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 256259_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256259_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256297_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256297_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
**** FOUND 07:38:26.27 -25:21:48.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256329_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256329_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256365_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
Preparing report for the candidate 256365_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
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Considering the candidate 256376_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256376_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
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Considering the candidate 256382_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 256382_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 211400_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 211400_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251853_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124
The candidate 251853_fd_Pup-02-Q1b1x1_2026-09-17_06-37-05_20.00sec_0.00C_LIGHTs_0124 did not pass the final checks
