This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje
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 11 03.4067 2461347.9067 12.84 08:29:24.57 -35:29:55.7
255.08652 2.04054 galactic Pyx Second-epoch detections are separated by 2.9" and 7.8 pix
The object was found in VSX 2" GDS_J0829244-352956
Type: M
# Max. Min./Amp. JD0 Period
14.850 r Y 3.290 r 383.500000000000 S
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:29:24.57 -35:29:55.7: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:29:24.57 -35:29:55.7: 14.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0829244-352956,2461347.9067,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0829244-352956 20261103.4067 12.84CV 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 11 03.4067 2461347.9067 13.23 08:24:42.83 -32:26:55.3
252.03461 3.01756 galactic Pup Second-epoch detections are separated by 1.6" and 8.6 pix
The object was found in VSX 3" GDS_J0824428-322651
Type: M
# Max. Min./Amp. JD0 Period
15.660 r Y 3.030 r 329.100000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:24:42.83 -32:26:55.3: 14.86 +/- 0.34 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:24:42.83 -32:26:55.3: 14.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.86 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0824428-322651,2461347.9067,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0824428-322651 20261103.4067 13.23CV 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 11 03.4067 2461347.9067 13.34 08:18:37.63 -33:38:15.3
252.28713 1.29226 galactic Pup Second-epoch detections are separated by 0.7" and 8.5 pix
The object was found in VSX 2" GDS_J0818375-333814
Type: VAR
# Max. Min./Amp. JD0 Period
13.510 r Y 0.710 r
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:18:37.63 -33:38:15.3: 14.28 +/- 0.21 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:18:37.63 -33:38:15.3: 14.42 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0818375-333814,2461347.9067,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0818375-333814 20261103.4067 13.34CV 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 11 03.4067 2461347.9067 13.54 08:12:41.58 -34:04:59.1
251.97115 0.02094 galactic Pup Second-epoch detections are separated by 3.3" and 8.6 pix
The object was found in VSX 4" GDS_J0812412-340459
Type: M
# Max. Min./Amp. JD0 Period
13.900 r Y 2.540 r 494.700000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:12:41.58 -34:04:59.1: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:12:41.58 -34:04:59.1: 14.83 +/- 0.35 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0812412-340459,2461347.9067,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0812412-340459 20261103.4067 13.54CV 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: 2461136.59122270 06.04.2026 02:11:11.641 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
First image: 2461136.59122270 06.04.2026 02:11:11.641 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Last image: 2461347.90711365 03.11.2026 09:46:04.619 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.26
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 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): 11869
Objects passed selection criteria: 11856
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 11109
Average stars matched: 10836.5 (97.547 %)
Memory usage VmPeak: 238268 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 04:19:45 CST 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: 2461136.59122270 06.04.2026 02:11:11.641 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
First image: 2461136.59122270 06.04.2026 02:11:11.641 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Last image: 2461347.90711365 03.11.2026 09:46:04.619 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.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.: -7.89
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: 51 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): 108673
Objects passed selection criteria: 108508
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 100115
Average stars matched: 96596.2 (96.4853 %)
Memory usage VmPeak: 507200 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 04:21:24 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
SExtractor catalog cache: saved Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461347.90624135
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits exists and is non-empty
wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits exists and is non-empty
wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (1st reference image)
verification OK: wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Image size: 937.3'x625.1' 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: 08:20:52.446 -34:00:38.17 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-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits (1st new image)
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
Image size: 939.8'x625.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 08:21:02.086 -34:01:44.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:20:52.446 -34:00:38.17
Second-epoch image center 08:21:02.086 -34:01:44.93
Angular distance between the image centers 0.0381 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits (2nd new image)
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Image size: 939.6'x625.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 08:20:58.662 -34:02:10.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:20:52.446 -34:00:38.17
Second-epoch image center 08:20:58.662 -34:02:10.64
Angular distance between the image centers 0.0335 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 08:21:02.086 -34:01:44.93
Second-epoch second image center 08:20:58.662 -34:02:10.64
Angular distance between the image centers 0.01381 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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits &> /tmp/tmp.kj8RZx6dpo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits &> /tmp/tmp.Q6Giobt7mf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits &> /tmp/tmp.JfyfkZ71Fe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits &> /tmp/tmp.prsSuJmhGP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Calibrating the magnitude scale
Found non-empty wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
Found non-empty wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
The reference image (wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits) and catalog (wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat) found
'wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat' -> 'wcsmag.cat'
Read 14942 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3301 to 135.2911 deg, Dec -39.2872 to -28.4077 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 115.3301 to 135.2911 deg, Dec -39.2872 to -28.4077 deg
Loaded 26003 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): 11585 out of 12071 total matches.
Matched with Tycho-2 12071 out of 14942 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.584300
a=0.000000 b=1.000000 c=22.584300
From vast_summary.log: estimated ref. image limiting mag.: -8.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.32
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 14942 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3301 to 135.2911 deg, Dec -39.2872 to -28.4077 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 115.3301 to 135.2911 deg, Dec -39.2872 to -28.4077 deg
Loaded 26003 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): 11585 out of 12071 total matches.
Matched with Tycho-2 12071 out of 14942 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Forced-photometry filter: calibrated wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits -> calib.txt_param_ref_wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (aperture=6.1)
Read 15218 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3104 to 135.2890 deg, Dec -39.2869 to -28.3706 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 115.3104 to 135.2890 deg, Dec -39.2869 to -28.3706 deg
Loaded 26108 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): 11747 out of 12249 total matches.
Matched with Tycho-2 12249 out of 15218 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Forced-photometry filter: calibrated wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits -> calib.txt_param_ref_wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
2.4 pix Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
2.4 pix fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
2.5 pix fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Limiting magnitude estimates:
14.3 mag. Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
14.3 mag. Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
14.0 mag. fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
14.0 mag. fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.kj8RZx6dpo (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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits' -> 'wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Checking if the catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat corresponding to the image wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat corresponding to the image wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS catalog name: wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=1211, bad_region=2731, passed=14942
Got 14942 stars (including 11158 good ones) from the SExtractor catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
util/solve_plate_with_UCAC5 got 14942 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 4866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 12846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 12846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 12846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 4862 stars left (next iteration limit 5351)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits N_match=4862 sigma_overall_arcsec=0.597 sigma_q1_arcsec=0.477 sigma_q2_arcsec=0.633 sigma_q3_arcsec=0.649 sigma_q4_arcsec=0.708 n_q1=1434 n_q2=838 n_q3=1638 n_q4=952 worst_quadrant_to_overall_ratio=1.185
WCS_HEADER_DIAG: file=Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits selection=current_pairs N_selected=4862 N_valid=4862 bias_ra_arcsec=0.009 bias_dec_arcsec=-0.008 median_sep_arcsec=0.440 p95_sep_arcsec=2.449 n_q1=1434 n_q2=838 n_q3=1638 n_q4=952 occupied_cells_4x4=16/16
The image catalog is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits -region wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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.Q6Giobt7mf (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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.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-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits' -> 'wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.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-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Checking if the catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat corresponding to the image wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat corresponding to the image wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS catalog name: wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=1268, bad_region=2796, passed=15218
Got 15218 stars (including 11355 good ones) from the SExtractor catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat
util/solve_plate_with_UCAC5 got 15218 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 13066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 13066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 13066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 4865 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits N_match=4865 sigma_overall_arcsec=0.587 sigma_q1_arcsec=0.482 sigma_q2_arcsec=0.642 sigma_q3_arcsec=0.637 sigma_q4_arcsec=0.718 n_q1=1431 n_q2=834 n_q3=1646 n_q4=954 worst_quadrant_to_overall_ratio=1.224
WCS_HEADER_DIAG: file=Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits selection=current_pairs N_selected=4865 N_valid=4865 bias_ra_arcsec=-0.008 bias_dec_arcsec=-0.007 median_sep_arcsec=0.446 p95_sep_arcsec=2.328 n_q1=1431 n_q2=834 n_q3=1646 n_q4=954 occupied_cells_4x4=16/16
The image catalog is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits -region wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.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.JfyfkZ71Fe (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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
WCS_IMAGE_NAME=wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
WCS-calibrated image found: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
Checking if the catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
WCS catalog name: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=823, bad_region=1672, passed=11707
Got 11707 stars (including 9279 good ones) from the SExtractor catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat
util/solve_plate_with_UCAC5 got 11707 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.8'
Seting catalog search parameters based on the expected field of view 939.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013053 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010442 (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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 4856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 10450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4858 matched stars entering correct_measured_positions(), 10450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 4858 matched stars entering correct_measured_positions(), 10450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 4858 stars left (next iteration limit 5337)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4858 robust_rms=6.454 arcsec worst_region_rms=11.463 arcsec outer_annulus_rms=11.463 arcsec
SIP_REFIT: SIP order 3 trial: matched=4858 robust_rms=1.074 arcsec worst_region_rms=1.694 arcsec outer_annulus_rms=1.292 arcsec
SIP_REFIT: SIP order 5 trial: matched=4858 robust_rms=0.774 arcsec worst_region_rms=1.011 arcsec outer_annulus_rms=1.011 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4858 robust_rms_before=2.018 arcsec robust_rms_before_corrected=0.712 arcsec robust_rms_after=0.774 arcsec worst_region_rms_before=1.137 worst_region_rms_after=1.011 outer_annulus_rms_before=3.436 outer_annulus_rms_after=1.011
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.sip_refit.4J1llP/candidate.fits
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.sip_refit.4J1llP/candidate.fits
Image size: 940.3'x625.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:21:02.150 -34:01:46.67 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 11707 stars ###
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.sip_refit.4J1llP/candidate.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction_3220099.cat.log'
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.sip_refit.4J1llP/candidate.wcscat.xy2sky.AAXMdx' -> 'vast_debug_catalog_after_xy2sky_correction_3220099.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 2.018 -> 0.774 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (cycle 1, search radius 3.9 arcsec, 4858 pairs from the previous 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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4651 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4651 pairs (4858 from the previous matching)
SIP_REFIT: SIP order 2 trial: matched=4651 robust_rms=6.323 arcsec worst_region_rms=10.864 arcsec outer_annulus_rms=10.864 arcsec
SIP_REFIT: SIP order 3 trial: matched=4651 robust_rms=1.055 arcsec worst_region_rms=1.661 arcsec outer_annulus_rms=1.264 arcsec
SIP_REFIT: SIP order 5 trial: matched=4651 robust_rms=0.754 arcsec worst_region_rms=0.996 arcsec outer_annulus_rms=0.996 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4651 robust_rms_before=0.754 arcsec robust_rms_before_corrected=0.754 arcsec robust_rms_after=0.754 arcsec worst_region_rms_before=1.000 worst_region_rms_after=0.996 outer_annulus_rms_before=1.000 outer_annulus_rms_after=0.996
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.sip_refit.DGNzWb/candidate.fits
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.sip_refit.DGNzWb/candidate.fits
Image size: 940.3'x625.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:21:02.150 -34:01:46.68 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 11707 stars ###
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.sip_refit.DGNzWb/candidate.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction_3220702.cat.log'
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.sip_refit.DGNzWb/candidate.wcscat.xy2sky.UGldEF' -> 'vast_debug_catalog_after_xy2sky_correction_3220702.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.754 -> 0.754 arcsec)
Accuracy estimation diagnostic: 4651 matched stars entering correct_measured_positions(), 10450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 4651 matched stars entering correct_measured_positions(), 10446 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
WCS_QUALITY_DIAG: file=fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits N_match=4651 sigma_overall_arcsec=0.765 sigma_q1_arcsec=0.799 sigma_q2_arcsec=0.966 sigma_q3_arcsec=0.705 sigma_q4_arcsec=0.805 n_q1=1380 n_q2=648 n_q3=1769 n_q4=854 worst_quadrant_to_overall_ratio=1.262
WCS_HEADER_DIAG: file=fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits selection=current_pairs N_selected=4651 N_valid=4651 bias_ra_arcsec=0.000 bias_dec_arcsec=-0.008 median_sep_arcsec=0.616 p95_sep_arcsec=1.699 n_q1=1380 n_q2=648 n_q3=1769 n_q4=854 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits -region wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.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.prsSuJmhGP (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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
WCS_IMAGE_NAME=wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
WCS-calibrated image found: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Checking if the catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
WCS catalog name: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=790, bad_region=1685, passed=11743
Got 11743 stars (including 9324 good ones) from the SExtractor catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat
util/solve_plate_with_UCAC5 got 11743 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.6'
Seting catalog search parameters based on the expected field of view 939.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013050 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010440 (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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 10463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 10463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 10463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 4850 stars left (next iteration limit 5331)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4850 robust_rms=6.620 arcsec worst_region_rms=12.148 arcsec outer_annulus_rms=12.148 arcsec
SIP_REFIT: SIP order 3 trial: matched=4850 robust_rms=0.932 arcsec worst_region_rms=1.230 arcsec outer_annulus_rms=1.225 arcsec
SIP_REFIT: SIP order 5 trial: matched=4850 robust_rms=0.772 arcsec worst_region_rms=1.043 arcsec outer_annulus_rms=1.043 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4850 robust_rms_before=2.050 arcsec robust_rms_before_corrected=0.723 arcsec robust_rms_after=0.772 arcsec worst_region_rms_before=1.173 worst_region_rms_after=1.043 outer_annulus_rms_before=3.061 outer_annulus_rms_after=1.043
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.sip_refit.pEp8pM/candidate.fits
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.sip_refit.pEp8pM/candidate.fits
Image size: 940.3'x625.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:20:58.739 -34:02:12.24 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 11743 stars ###
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.sip_refit.pEp8pM/candidate.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction_3220096.cat.log'
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.sip_refit.pEp8pM/candidate.wcscat.xy2sky.6bZ4b7' -> 'vast_debug_catalog_after_xy2sky_correction_3220096.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 2.050 -> 0.772 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (cycle 1, search radius 3.9 arcsec, 4850 pairs from the previous 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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4652 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4652 pairs (4850 from the previous matching)
SIP_REFIT: SIP order 2 trial: matched=4652 robust_rms=6.480 arcsec worst_region_rms=11.533 arcsec outer_annulus_rms=11.533 arcsec
SIP_REFIT: SIP order 3 trial: matched=4652 robust_rms=0.915 arcsec worst_region_rms=1.200 arcsec outer_annulus_rms=1.200 arcsec
SIP_REFIT: SIP order 5 trial: matched=4652 robust_rms=0.758 arcsec worst_region_rms=1.037 arcsec outer_annulus_rms=1.037 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4652 robust_rms_before=0.758 arcsec robust_rms_before_corrected=0.758 arcsec robust_rms_after=0.758 arcsec worst_region_rms_before=1.037 worst_region_rms_after=1.037 outer_annulus_rms_before=1.037 outer_annulus_rms_after=1.037
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.sip_refit.wtMu2V/candidate.fits
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.sip_refit.wtMu2V/candidate.fits
Image size: 940.3'x625.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:20:58.739 -34:02:12.25 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 11743 stars ###
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.sip_refit.wtMu2V/candidate.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction_3220705.cat.log'
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.sip_refit.wtMu2V/candidate.wcscat.xy2sky.Q8i12e' -> 'vast_debug_catalog_after_xy2sky_correction_3220705.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.758 -> 0.758 arcsec)
Accuracy estimation diagnostic: 4652 matched stars entering correct_measured_positions(), 10463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 4652 matched stars entering correct_measured_positions(), 10462 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
WCS_QUALITY_DIAG: file=fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits N_match=4652 sigma_overall_arcsec=0.746 sigma_q1_arcsec=0.805 sigma_q2_arcsec=0.952 sigma_q3_arcsec=0.697 sigma_q4_arcsec=0.810 n_q1=1394 n_q2=655 n_q3=1753 n_q4=850 worst_quadrant_to_overall_ratio=1.276
WCS_HEADER_DIAG: file=fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits selection=current_pairs N_selected=4652 N_valid=4652 bias_ra_arcsec=-0.007 bias_dec_arcsec=-0.001 median_sep_arcsec=0.605 p95_sep_arcsec=1.708 n_q1=1394 n_q2=655 n_q3=1753 n_q4=850 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits -region wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits to local_wcs_cache/
'wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits'
Saving the final (post-refit) wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits to local_wcs_cache/
'wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits'
Saving the final (post-refit) wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits to local_wcs_cache/
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits' -> 'local_wcs_cache/wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits'
Saving the final (post-refit) wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits to local_wcs_cache/
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits' -> 'local_wcs_cache/wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits sigma_overall=0.597 worst_q_ratio=1.185
ref2=Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits sigma_overall=0.587 worst_q_ratio=1.224
new1=fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits sigma_overall=0.765 worst_q_ratio=1.262
new2=fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits sigma_overall=0.746 worst_q_ratio=1.276
reference average sigma_overall=0.592 worst_q_ratio=1.2045
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010_astrometric_residuals.png (4862 matched stars from wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.55 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011_astrometric_residuals.png (4865 matched stars from wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.55 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510_astrometric_residuals.png (4651 matched stars from wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511_astrometric_residuals.png (4652 matched stars from wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits'
Saving fully-calibrated image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits'
Preparing the HTML report for the field Pup-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:18:22.24 -30:39:44.0: 11.07 +/- 0.01 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:13:11.54 -31:53:54.4: 11.21 +/- 0.01 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:20:09.36 -29:54:52.7: 11.34 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:04:46.20 -32:30:11.4: 11.21 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:58:56.12 -32:51:57.7: 11.71 +/- 0.03 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:21:10.00 -32:33:09.5: 11.53 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:20:09.36 -29:54:52.7: 11.33 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:58:56.12 -32:51:57.7: 11.67 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:04:46.20 -32:30:11.4: 11.17 +/- 0.01 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:21:10.00 -32:33:09.5: 11.54 +/- 0.02 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:13:11.54 -31:53:54.4: 11.24 +/- 0.01 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:18:22.24 -30:39:44.0: 11.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.01
Forced photometry reference-image weighted average: 11.69 +/- 0.02
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Forced photometry reference-image weighted average: 11.18 +/- 0.01
Forced photometry reference-image weighted average: 11.07 +/- 0.01
Forced photometry filter REJECTED candidate at 07:58:56.12 -32:51:57.7: ref_mag=11.69 +/- 0.02 new_mean_mag=11.1460 delta=0.54 (need > 0.90)
Forced photometry reference-image weighted average: 11.22 +/- 0.01
Forced photometry filter REJECTED candidate at 08:20:09.36 -29:54:52.7: ref_mag=11.34 +/- 0.01 new_mean_mag=11.2961 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:21:10.00 -32:33:09.5: ref_mag=11.53 +/- 0.01 new_mean_mag=11.1333 delta=0.40 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:04:46.20 -32:30:11.4: ref_mag=11.18 +/- 0.01 new_mean_mag=11.1715 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:18:22.24 -30:39:44.0: ref_mag=11.07 +/- 0.01 new_mean_mag=11.0537 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:13:11.54 -31:53:54.4: ref_mag=11.22 +/- 0.01 new_mean_mag=11.1620 delta=0.06 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20914_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 20914_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:08:56.60 -37:28:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20949_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 20949_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:04:27.22 -35:15:12.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20962_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 20962_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:23:19.17 -35:24:57.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20973_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 20973_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20978_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 20978_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20979_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 20979_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20983_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 20983_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20986_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 20986_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20993_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 20993_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
SExtractor catalog cache: saved Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Creating symlink local_wcs_cache/wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Creating symlink local_wcs_cache/wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
Creating symlink local_wcs_cache/wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Checking 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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits exists and is non-empty
wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits exists and is non-empty
wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (1st reference image)
verification OK: wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Image size: 937.3'x625.1' 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: 08:20:52.446 -34:00:38.17 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-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits (1st new image)
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
Image size: 940.3'x625.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:21:02.150 -34:01:46.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:20:52.446 -34:00:38.17
Second-epoch image center 08:21:02.150 -34:01:46.68
Angular distance between the image centers 0.0385 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits (2nd new image)
verification OK: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Image size: 940.3'x625.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:20:58.739 -34:02:12.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:20:52.446 -34:00:38.17
Second-epoch image center 08:20:58.739 -34:02:12.25
Angular distance between the image centers 0.0340 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 08:21:02.150 -34:01:46.68
Second-epoch second image center 08:20:58.739 -34:02:12.25
Angular distance between the image centers 0.01375 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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits &> /tmp/tmp.cLeuJk9IcD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits &> /tmp/tmp.rUoFgr2sZ4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits &> /tmp/tmp.4rMN8rLKsF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits &> /tmp/tmp.sz4pu73tSq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Calibrating the magnitude scale
Found non-empty wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
Found non-empty wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits and wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
The reference image (wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits) and catalog (wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat) found
'wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat' -> 'wcsmag.cat'
Read 132037 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3025 to 135.3575 deg, Dec -39.2952 to -28.3517 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 115.3025 to 135.3575 deg, Dec -39.2952 to -28.3517 deg
Loaded 26236 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): 17756 out of 21157 total matches.
Matched with Tycho-2 21157 out of 132037 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.381200
a=0.000000 b=1.000000 c=22.381200
From vast_summary.log: estimated ref. image limiting mag.: -7.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.49
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 132037 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3025 to 135.3575 deg, Dec -39.2952 to -28.3517 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 115.3025 to 135.3575 deg, Dec -39.2952 to -28.3517 deg
Loaded 26236 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): 17756 out of 21157 total matches.
Matched with Tycho-2 21157 out of 132037 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Forced-photometry filter: calibrated wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits -> calib.txt_param_ref_wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (aperture=4.5)
Read 134376 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.3028 to 135.3209 deg, Dec -39.2901 to -28.3510 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 115.3028 to 135.3209 deg, Dec -39.2901 to -28.3510 deg
Loaded 26201 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): 17706 out of 21125 total matches.
Matched with Tycho-2 21125 out of 134376 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Forced-photometry filter: calibrated wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits -> calib.txt_param_ref_wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 79 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
2.1 pix Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
2.4 pix fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
2.5 pix fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Limiting magnitude estimates:
14.5 mag. Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
14.5 mag. Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
14.1 mag. fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
14.1 mag. fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.cLeuJk9IcD (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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits' -> 'wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
Checking if the catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat corresponding to the image wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat corresponding to the image wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits
WCS catalog name: wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=12, blended=12979, bad_region=16456, passed=132025
Got 132025 stars (including 104056 good ones) from the SExtractor catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat
util/solve_plate_with_UCAC5 got 132025 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 4882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 120193 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 120193 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 120193 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 4883 stars left (next iteration limit 5370)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits N_match=4883 sigma_overall_arcsec=0.592 sigma_q1_arcsec=0.472 sigma_q2_arcsec=0.621 sigma_q3_arcsec=0.637 sigma_q4_arcsec=0.711 n_q1=1494 n_q2=865 n_q3=1581 n_q4=943 worst_quadrant_to_overall_ratio=1.201
WCS_HEADER_DIAG: file=Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits selection=current_pairs N_selected=4883 N_valid=4883 bias_ra_arcsec=0.025 bias_dec_arcsec=0.003 median_sep_arcsec=0.436 p95_sep_arcsec=2.106 n_q1=1494 n_q2=865 n_q3=1581 n_q4=943 occupied_cells_4x4=16/16
The image catalog is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits -region wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.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.rUoFgr2sZ4 (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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.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-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits' -> 'wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.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-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
Checking if the catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat corresponding to the image wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat corresponding to the image wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits
WCS catalog name: wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=17, blended=13323, bad_region=16854, passed=134359
Got 134359 stars (including 105688 good ones) from the SExtractor catalog wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat
util/solve_plate_with_UCAC5 got 134359 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 4876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 122212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 122212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 122211 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 4875 stars left (next iteration limit 5362)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.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-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits N_match=4875 sigma_overall_arcsec=0.584 sigma_q1_arcsec=0.483 sigma_q2_arcsec=0.608 sigma_q3_arcsec=0.639 sigma_q4_arcsec=0.714 n_q1=1508 n_q2=864 n_q3=1564 n_q4=939 worst_quadrant_to_overall_ratio=1.223
WCS_HEADER_DIAG: file=Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits selection=current_pairs N_selected=4875 N_valid=4875 bias_ra_arcsec=0.007 bias_dec_arcsec=-0.001 median_sep_arcsec=0.442 p95_sep_arcsec=2.095 n_q1=1508 n_q2=864 n_q3=1564 n_q4=939 occupied_cells_4x4=16/16
The image catalog is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits -region wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.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.4rMN8rLKsF (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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
WCS_IMAGE_NAME=wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
WCS-calibrated image found: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
Checking if the catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
WCS catalog name: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=7575, bad_region=9561, passed=95042
Got 95042 stars (including 78323 good ones) from the SExtractor catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat
util/solve_plate_with_UCAC5 got 95042 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.3'
Seting catalog search parameters based on the expected field of view 940.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013060 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010448 (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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 4866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 88181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 88181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 88181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 4863 stars left (next iteration limit 5352)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.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=4863 robust_rms=6.501 arcsec worst_region_rms=10.320 arcsec outer_annulus_rms=10.320 arcsec
SIP_REFIT: SIP order 3 trial: matched=4863 robust_rms=1.068 arcsec worst_region_rms=1.673 arcsec outer_annulus_rms=1.283 arcsec
SIP_REFIT: SIP order 5 trial: matched=4863 robust_rms=0.766 arcsec worst_region_rms=0.996 arcsec outer_annulus_rms=0.996 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4863 robust_rms_before=0.763 arcsec robust_rms_before_corrected=0.721 arcsec robust_rms_after=0.766 arcsec worst_region_rms_before=0.999 worst_region_rms_after=0.996 outer_annulus_rms_before=0.999 outer_annulus_rms_after=0.996
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.999 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits worst_region_rms_kept=0.999 arcsec robust_rms_kept=0.721 arcsec matched=4863
WCS_QUALITY_DIAG: file=fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits N_match=4863 sigma_overall_arcsec=0.721 sigma_q1_arcsec=0.739 sigma_q2_arcsec=0.705 sigma_q3_arcsec=0.726 sigma_q4_arcsec=0.838 n_q1=1496 n_q2=674 n_q3=1796 n_q4=897 worst_quadrant_to_overall_ratio=1.162
WCS_HEADER_DIAG: file=fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits selection=current_pairs N_selected=4863 N_valid=4863 bias_ra_arcsec=0.008 bias_dec_arcsec=0.007 median_sep_arcsec=0.630 p95_sep_arcsec=2.456 n_q1=1496 n_q2=674 n_q3=1796 n_q4=897 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits -region wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.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.sz4pu73tSq (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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
WCS_IMAGE_NAME=wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
WCS-calibrated image found: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Checking if the catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits alredy exist and is non-empty...
Catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat corresponding to the image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
WCS catalog name: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=4, blended=7514, bad_region=9575, passed=93843
Got 93843 stars (including 77129 good ones) from the SExtractor catalog wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat
util/solve_plate_with_UCAC5 got 93843 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.3'
Seting catalog search parameters based on the expected field of view 940.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013060 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010448 (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 253 to 309 (Dec -39.3 to -28.5)
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: 4868 matched stars entering correct_measured_positions(), 4869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 86952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 86952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 86952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 4868 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.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=4868 robust_rms=6.614 arcsec worst_region_rms=11.654 arcsec outer_annulus_rms=11.654 arcsec
SIP_REFIT: SIP order 3 trial: matched=4868 robust_rms=0.936 arcsec worst_region_rms=1.233 arcsec outer_annulus_rms=1.222 arcsec
SIP_REFIT: SIP order 5 trial: matched=4868 robust_rms=0.774 arcsec worst_region_rms=1.057 arcsec outer_annulus_rms=1.057 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4868 robust_rms_before=0.775 arcsec robust_rms_before_corrected=0.727 arcsec robust_rms_after=0.774 arcsec worst_region_rms_before=1.052 worst_region_rms_after=1.057 outer_annulus_rms_before=1.052 outer_annulus_rms_after=1.057
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 1.052 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits worst_region_rms_kept=1.052 arcsec robust_rms_kept=0.727 arcsec matched=4868
WCS_QUALITY_DIAG: file=fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits N_match=4868 sigma_overall_arcsec=0.710 sigma_q1_arcsec=0.713 sigma_q2_arcsec=0.769 sigma_q3_arcsec=0.701 sigma_q4_arcsec=0.857 n_q1=1508 n_q2=685 n_q3=1779 n_q4=896 worst_quadrant_to_overall_ratio=1.207
WCS_HEADER_DIAG: file=fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits selection=current_pairs N_selected=4868 N_valid=4868 bias_ra_arcsec=-0.001 bias_dec_arcsec=0.001 median_sep_arcsec=0.625 p95_sep_arcsec=2.530 n_q1=1508 n_q2=685 n_q3=1779 n_q4=896 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits -region wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.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-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-44-49_20.00sec_-0.00C_LIGHT_0510.fits
Saving fully-calibrated image wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.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_2026-11-03_CI_Pup-04-Q2b1x1_041423_TTUQ2b1x1_3089234_gu6Deeje/wcs_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511.fits
Preparing the HTML report for the field Pup-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:36:08.41 -31:34:34.1: 13.37 +/- 0.09 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:19:58.83 -30:30:32.9: 13.71 +/- 0.12 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:10:17.71 -31:07:34.6: 13.09 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:56:14.06 -30:01:21.7: 13.59 +/- 0.17 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:11:41.61 -31:06:27.5: 13.55 +/- 0.11 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:12:52.44 -29:48:28.3: 13.59 +/- 0.11 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:14:15.94 -34:15:31.0: 13.48 +/- 0.11 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:10:20.30 -31:15:42.6: 13.88 +/- 0.16 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:06:07.04 -30:41:35.8: 13.95 +/- 0.18 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:54:47.47 -37:17:15.0: 13.58 +/- 0.13 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:06:07.04 -30:41:35.8: 13.78 +/- 0.15 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:12:52.44 -29:48:28.3: 13.65 +/- 0.11 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:10:17.71 -31:07:34.6: 13.15 +/- 0.08 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:19:58.83 -30:30:32.9: 13.76 +/- 0.13 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:56:14.06 -30:01:21.7: 13.57 +/- 0.16 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:54:47.47 -37:17:15.0: 13.28 +/- 0.10 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:10:20.30 -31:15:42.6: 13.63 +/- 0.12 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:11:41.61 -31:06:27.5: 13.72 +/- 0.13 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:36:08.41 -31:34:34.1: 13.28 +/- 0.08 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:14:15.94 -34:15:31.0: 13.88 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.08
Forced photometry reference-image weighted average: 13.85 +/- 0.12
Forced photometry reference-image weighted average: 13.12 +/- 0.05
Forced photometry reference-image weighted average: 13.73 +/- 0.09
Forced photometry reference-image weighted average: 13.58 +/- 0.12
Forced photometry reference-image weighted average: 13.38 +/- 0.08
Forced photometry filter REJECTED candidate at 08:12:52.44 -29:48:28.3: ref_mag=13.62 +/- 0.08 new_mean_mag=13.6134 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:06:07.04 -30:41:35.8: ref_mag=13.85 +/- 0.12 new_mean_mag=13.6086 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 13.32 +/- 0.06
Forced photometry filter REJECTED candidate at 08:10:17.71 -31:07:34.6: ref_mag=13.12 +/- 0.05 new_mean_mag=13.4310 delta=-0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:19:58.83 -30:30:32.9: ref_mag=13.73 +/- 0.09 new_mean_mag=13.6282 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:56:14.06 -30:01:21.7: ref_mag=13.58 +/- 0.12 new_mean_mag=13.6008 delta=-0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:54:47.47 -37:17:15.0: ref_mag=13.38 +/- 0.08 new_mean_mag=13.3995 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.62 +/- 0.09
Forced photometry reference-image weighted average: 13.72 +/- 0.10
Forced photometry reference-image weighted average: 13.62 +/- 0.08
Forced photometry filter REJECTED candidate at 08:36:08.41 -31:34:34.1: ref_mag=13.32 +/- 0.06 new_mean_mag=13.4989 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:14:15.94 -34:15:31.0: ref_mag=13.62 +/- 0.09 new_mean_mag=13.8205 delta=-0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:10:20.30 -31:15:42.6: ref_mag=13.72 +/- 0.10 new_mean_mag=13.5293 delta=0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:11:41.61 -31:06:27.5: ref_mag=13.62 +/- 0.08 new_mean_mag=13.4760 delta=0.14 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:56:23.50 -30:06:30.1: 13.72 +/- 0.17 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:57:13.99 -33:24:01.3: 13.05 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:09:37.02 -34:50:51.8: 12.84 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:09:40.19 -30:26:05.6: 12.98 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:08:51.39 -34:01:34.3: 13.21 +/- 0.09 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:54:03.94 -30:02:43.8: 13.75 +/- 0.15 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:01:38.91 -33:18:39.4: 13.48 +/- 0.10 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:59:09.80 -31:33:49.0: 13.04 +/- 0.08 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:15:41.85 -32:24:50.1: 12.83 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:56:23.50 -30:06:30.1: 13.53 +/- 0.14 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:09:37.02 -34:50:51.8: 12.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.11
Forced photometry filter REJECTED candidate at 07:56:23.50 -30:06:30.1: ref_mag=13.61 +/- 0.11 new_mean_mag=13.6054 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.86 +/- 0.04
Forced photometry filter REJECTED candidate at 08:09:37.02 -34:50:51.8: ref_mag=12.86 +/- 0.04 new_mean_mag=13.0467 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:57:13.99 -33:24:01.3: 13.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.05
Forced photometry filter REJECTED candidate at 07:57:13.99 -33:24:01.3: ref_mag=13.07 +/- 0.05 new_mean_mag=13.1465 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:08:51.39 -34:01:34.3: 13.36 +/- 0.10 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:09:40.19 -30:26:05.6: 12.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.07
Forced photometry filter REJECTED candidate at 08:08:51.39 -34:01:34.3: ref_mag=13.28 +/- 0.07 new_mean_mag=13.1260 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.94 +/- 0.05
Forced photometry filter REJECTED candidate at 08:09:40.19 -30:26:05.6: ref_mag=12.94 +/- 0.05 new_mean_mag=12.9303 delta=0.01 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:01:38.91 -33:18:39.4: 13.50 +/- 0.11 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:55:13.11 -30:38:26.5: 12.84 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:15:41.85 -32:24:50.1: 12.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.07
Forced photometry filter REJECTED candidate at 08:01:38.91 -33:18:39.4: ref_mag=13.49 +/- 0.07 new_mean_mag=13.3608 delta=0.13 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:54:03.94 -30:02:43.8: 13.63 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.04
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:59:09.80 -31:33:49.0: 13.15 +/- 0.09 detection
Forced photometry filter REJECTED candidate at 08:15:41.85 -32:24:50.1: ref_mag=12.85 +/- 0.04 new_mean_mag=13.0383 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.68 +/- 0.10
Forced photometry filter REJECTED candidate at 07:54:03.94 -30:02:43.8: ref_mag=13.68 +/- 0.10 new_mean_mag=13.5133 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 13.09 +/- 0.06
Forced photometry filter REJECTED candidate at 07:59:09.80 -31:33:49.0: ref_mag=13.09 +/- 0.06 new_mean_mag=13.1025 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:55:13.11 -30:38:26.5: 12.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.04
Forced photometry filter REJECTED candidate at 07:55:13.11 -30:38:26.5: ref_mag=12.83 +/- 0.04 new_mean_mag=13.0689 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:56:33.70 -30:06:21.2: 13.06 +/- 0.08 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:48:07.73 -36:43:47.9: 13.21 +/- 0.10 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:05:57.52 -30:56:19.7: 12.85 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:56:23.20 -30:03:49.4: 12.91 +/- 0.11 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:59:46.33 -31:07:00.2: 12.48 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:17:07.47 -31:26:37.6: 10.96 +/- 0.01 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:07:08.49 -36:38:45.6: 12.57 +/- 0.05 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:56:33.70 -30:06:21.2: 13.01 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.06
Forced photometry filter REJECTED candidate at 07:56:33.70 -30:06:21.2: ref_mag=13.03 +/- 0.06 new_mean_mag=13.0314 delta=0.00 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:48:07.73 -36:43:47.9: 13.19 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.07
Forced photometry filter REJECTED candidate at 07:48:07.73 -36:43:47.9: ref_mag=13.20 +/- 0.07 new_mean_mag=12.7575 delta=0.44 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:56:23.20 -30:03:49.4: 12.92 +/- 0.11 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:05:57.52 -30:56:19.7: 12.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.08
Forced photometry filter REJECTED candidate at 07:56:23.20 -30:03:49.4: ref_mag=12.92 +/- 0.08 new_mean_mag=12.9984 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.83 +/- 0.04
Forced photometry filter REJECTED candidate at 08:05:57.52 -30:56:19.7: ref_mag=12.83 +/- 0.04 new_mean_mag=12.8370 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:59:46.33 -31:07:00.2: 12.45 +/- 0.04 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:07:08.49 -36:38:45.6: 12.54 +/- 0.05 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:17:07.47 -31:26:37.6: 10.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.03
Forced photometry reference-image weighted average: 12.55 +/- 0.03
Forced photometry reference-image weighted average: 10.98 +/- 0.01
Forced photometry filter REJECTED candidate at 07:59:46.33 -31:07:00.2: ref_mag=12.46 +/- 0.03 new_mean_mag=12.5727 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:07:08.49 -36:38:45.6: ref_mag=12.55 +/- 0.03 new_mean_mag=12.4583 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:17:07.47 -31:26:37.6: ref_mag=10.98 +/- 0.01 new_mean_mag=12.5584 delta=-1.58 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:08:10.41 -36:24:16.6: 12.70 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:01:58.44 -35:08:26.8: 12.62 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:16:59.59 -32:59:54.4: 12.81 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:54:14.61 -32:36:07.3: 13.20 +/- 0.09 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:02:58.25 -31:50:17.1: 13.12 +/- 0.09 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:29:24.57 -35:29:55.7: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:01:38.68 -30:31:46.5: 13.21 +/- 0.09 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:50:27.34 -34:36:41.3: 13.26 +/- 0.10 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:08:10.41 -36:24:16.6: 12.68 +/- 0.06 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:03:42.86 -31:44:33.8: 13.69 +/- 0.16 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:24:42.83 -32:26:55.3: 14.86 +/- 0.34 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.04
Forced photometry filter REJECTED candidate at 08:08:10.41 -36:24:16.6: ref_mag=12.69 +/- 0.04 new_mean_mag=12.6457 delta=0.04 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:01:58.44 -35:08:26.8: 12.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.04
Forced photometry filter REJECTED candidate at 08:01:58.44 -35:08:26.8: ref_mag=12.67 +/- 0.04 new_mean_mag=12.5750 delta=0.09 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:16:59.59 -32:59:54.4: 12.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.05
Forced photometry filter REJECTED candidate at 08:16:59.59 -32:59:54.4: ref_mag=12.87 +/- 0.05 new_mean_mag=12.9143 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:54:14.61 -32:36:07.3: 13.08 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.06
Forced photometry filter REJECTED candidate at 07:54:14.61 -32:36:07.3: ref_mag=13.13 +/- 0.06 new_mean_mag=13.1129 delta=0.02 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:02:58.25 -31:50:17.1: 13.05 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.06
Forced photometry filter REJECTED candidate at 08:02:58.25 -31:50:17.1: ref_mag=13.08 +/- 0.06 new_mean_mag=13.0180 delta=0.06 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:29:24.57 -35:29:55.7: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:01:38.68 -30:31:46.5: 13.26 +/- 0.09 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:50:27.34 -34:36:41.3: 13.22 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.06
Forced photometry filter REJECTED candidate at 08:01:38.68 -30:31:46.5: ref_mag=13.23 +/- 0.06 new_mean_mag=13.2566 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.24 +/- 0.07
Forced photometry filter REJECTED candidate at 07:50:27.34 -34:36:41.3: ref_mag=13.24 +/- 0.07 new_mean_mag=13.0548 delta=0.19 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:24:42.83 -32:26:55.3: 14.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.86 +/- 0.34
Forced photometry filter KEPT candidate at 08:24:42.83 -32:26:55.3: ref_mag=14.86 +/- 0.34 new_mean_mag=13.2307 delta=1.63 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:03:42.86 -31:44:33.8: 13.42 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.10
Forced photometry filter REJECTED candidate at 08:03:42.86 -31:44:33.8: ref_mag=13.52 +/- 0.10 new_mean_mag=13.3129 delta=0.21 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:18:37.63 -33:38:15.3: 14.28 +/- 0.21 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:52:31.35 -32:06:18.3: 13.55 +/- 0.14 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:47:39.37 -35:32:22.1: 13.63 +/- 0.14 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:17:05.19 -31:25:19.3: 12.69 +/- 0.07 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:37:08.28 -31:23:45.5: 13.66 +/- 0.13 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:56:14.37 -30:14:48.8: 13.58 +/- 0.14 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:18:37.63 -33:38:15.3: 14.42 +/- 0.23 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:22:41.07 -30:25:39.8: 13.32 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.15
Forced photometry filter KEPT candidate at 08:18:37.63 -33:38:15.3: ref_mag=14.34 +/- 0.15 new_mean_mag=13.3220 delta=1.01 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:07:17.15 -29:48:27.5: 14.09 +/- 0.22 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:52:31.35 -32:06:18.3: 13.77 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.11
Forced photometry filter REJECTED candidate at 07:52:31.35 -32:06:18.3: ref_mag=13.64 +/- 0.11 new_mean_mag=13.5269 delta=0.11 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:17:05.19 -31:25:19.3: 12.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.04
Forced photometry filter REJECTED candidate at 08:17:05.19 -31:25:19.3: ref_mag=12.65 +/- 0.04 new_mean_mag=13.4856 delta=-0.84 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:47:39.37 -35:32:22.1: 13.71 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.10
Forced photometry filter REJECTED candidate at 07:47:39.37 -35:32:22.1: ref_mag=13.67 +/- 0.10 new_mean_mag=13.4962 delta=0.17 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:37:08.28 -31:23:45.5: 13.76 +/- 0.13 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:56:14.37 -30:14:48.8: 13.63 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.09
Forced photometry filter REJECTED candidate at 08:37:08.28 -31:23:45.5: ref_mag=13.71 +/- 0.09 new_mean_mag=13.4194 delta=0.29 (need > 0.90)
Forced photometry reference-image weighted average: 13.60 +/- 0.10
Forced photometry filter REJECTED candidate at 07:56:14.37 -30:14:48.8: ref_mag=13.60 +/- 0.10 new_mean_mag=13.5164 delta=0.09 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:22:41.07 -30:25:39.8: 13.37 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.07
Forced photometry filter REJECTED candidate at 08:22:41.07 -30:25:39.8: ref_mag=13.34 +/- 0.07 new_mean_mag=13.2882 delta=0.05 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:07:17.15 -29:48:27.5: 14.26 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.17
Forced photometry filter REJECTED candidate at 08:07:17.15 -29:48:27.5: ref_mag=14.16 +/- 0.17 new_mean_mag=13.7456 delta=0.41 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:59:35.88 -34:49:42.5: 13.76 +/- 0.14 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:00:01.01 -30:04:04.4: 13.87 +/- 0.19 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:51:17.29 -30:33:44.5: 14.03 +/- 0.19 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:54:54.73 -34:49:22.0: 13.96 +/- 0.18 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:10:15.00 -29:57:55.8: 13.78 +/- 0.14 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:56:14.39 -30:57:14.9: 13.67 +/- 0.13 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:55:40.03 -30:24:15.1: 14.02 +/- 0.18 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:59:35.88 -34:49:42.5: 13.88 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.10
Forced photometry filter REJECTED candidate at 07:59:35.88 -34:49:42.5: ref_mag=13.81 +/- 0.10 new_mean_mag=13.4904 delta=0.32 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:54:54.73 -34:49:22.0: 13.96 +/- 0.18 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:51:17.29 -30:33:44.5: 13.89 +/- 0.16 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:00:01.01 -30:04:04.4: 13.90 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.12
Forced photometry reference-image weighted average: 13.96 +/- 0.13
Forced photometry reference-image weighted average: 13.89 +/- 0.13
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:10:15.00 -29:57:55.8: 13.67 +/- 0.12 detection
Forced photometry filter REJECTED candidate at 07:51:17.29 -30:33:44.5: ref_mag=13.95 +/- 0.12 new_mean_mag=13.8240 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:00:01.01 -30:04:04.4: ref_mag=13.89 +/- 0.13 new_mean_mag=13.7683 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:54:54.73 -34:49:22.0: ref_mag=13.96 +/- 0.13 new_mean_mag=13.6385 delta=0.32 (need > 0.90)
Forced photometry reference-image weighted average: 13.71 +/- 0.09
Forced photometry filter REJECTED candidate at 08:10:15.00 -29:57:55.8: ref_mag=13.71 +/- 0.09 new_mean_mag=13.5668 delta=0.15 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:56:14.39 -30:57:14.9: 13.80 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.10
Forced photometry filter REJECTED candidate at 07:56:14.39 -30:57:14.9: ref_mag=13.73 +/- 0.10 new_mean_mag=13.7584 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:55:40.03 -30:24:15.1: 13.79 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.11
Forced photometry filter REJECTED candidate at 07:55:40.03 -30:24:15.1: ref_mag=13.87 +/- 0.11 new_mean_mag=13.8477 delta=0.03 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:03:35.52 -32:51:28.1: 14.04 +/- 0.17 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:10:23.86 -30:38:23.6: 13.95 +/- 0.16 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:11:08.98 -33:16:04.4: 13.91 +/- 0.15 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 07:55:35.35 -32:17:20.5: 14.29 +/- 0.24 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:06:16.01 -31:05:38.3: 14.13 +/- 0.18 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:11:01.20 -32:16:13.7: 13.79 +/- 0.15 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:03:35.52 -32:51:28.1: 14.46 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.14
Forced photometry filter REJECTED candidate at 08:03:35.52 -32:51:28.1: ref_mag=14.17 +/- 0.14 new_mean_mag=13.7237 delta=0.45 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:12:41.58 -34:04:59.1: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:10:23.86 -30:38:23.6: 13.86 +/- 0.15 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:11:08.98 -33:16:04.4: 13.79 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.11
Forced photometry reference-image weighted average: 13.84 +/- 0.10
Forced photometry filter REJECTED candidate at 08:10:23.86 -30:38:23.6: ref_mag=13.90 +/- 0.11 new_mean_mag=13.6956 delta=0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:11:08.98 -33:16:04.4: ref_mag=13.84 +/- 0.10 new_mean_mag=13.6346 delta=0.20 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 07:55:35.35 -32:17:20.5: 14.15 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.16
Forced photometry filter REJECTED candidate at 07:55:35.35 -32:17:20.5: ref_mag=14.21 +/- 0.16 new_mean_mag=13.7231 delta=0.49 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:06:16.01 -31:05:38.3: 13.88 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.11
Forced photometry filter REJECTED candidate at 08:06:16.01 -31:05:38.3: ref_mag=13.97 +/- 0.11 new_mean_mag=13.6965 delta=0.28 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:11:01.20 -32:16:13.7: 13.74 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.10
Forced photometry filter REJECTED candidate at 08:11:01.20 -32:16:13.7: ref_mag=13.76 +/- 0.10 new_mean_mag=13.6886 delta=0.07 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:12:41.58 -34:04:59.1: 14.83 +/- 0.35 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.35
Forced photometry filter KEPT candidate at 08:12:41.58 -34:04:59.1: ref_mag=14.83 +/- 0.35 new_mean_mag=13.5312 delta=1.30 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:10:02.55 -33:08:30.7: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-11-11_20.00sec_-4.90C_LIGHT_0010.fits at 08:04:14.81 -33:44:04.4: 13.98 +/- 0.16 detection
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:10:02.55 -33:08:30.7: 14.55 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.25
Forced photometry filter REJECTED candidate at 08:10:02.55 -33:08:30.7: ref_mag=14.55 +/- 0.25 new_mean_mag=13.6779 delta=0.87 (need > 0.90)
Forced photometry on wcs_Pup-04-Q2b1x1_2026-04-05_21-12-02_20.00sec_-4.90C_LIGHT_0011.fits at 08:04:14.81 -33:44:04.4: 14.40 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.13
Forced photometry filter REJECTED candidate at 08:04:14.81 -33:44:04.4: ref_mag=14.11 +/- 0.13 new_mean_mag=13.7971 delta=0.32 (need > 0.90)
Adding exclusion_list_local.txt__out154776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155143.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 58s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 154220_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154220_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154221_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154221_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154237_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154237_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154249_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154249_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154251_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154251_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154254_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154254_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154259_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154259_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154265_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154265_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154270_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154270_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154276_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154276_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154279_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154279_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154283_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154283_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154293_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154293_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154304_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154304_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154309_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154309_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154317_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154317_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 07:57:01.61 -32:06:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154319_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154319_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154320_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154320_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154324_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154324_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154325_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154325_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154327_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154327_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154338_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154338_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154340_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154340_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154343_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154343_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154344_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154344_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154352_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154352_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154353_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154353_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154356_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154356_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 07:52:58.15 -33:20:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154361_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154361_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154365_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154365_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:26:13.06 -32:57:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154458_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154458_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:07:50.02 -35:54:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154514_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154514_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:06:08.35 -37:17:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154535_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154535_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:21:22.77 -33:05:11.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154552_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154552_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:30:39.07 -31:20:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154585_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154585_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:20:21.07 -32:13:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154588_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154588_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:10:48.99 -32:52:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154606_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154606_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154686_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154686_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154688_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154688_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:23:05.04 -33:52:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154700_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154700_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:39:58.15 -34:01:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154753_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154753_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154762_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154762_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154771_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154771_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154776_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
Preparing report for the candidate 154776_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
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Considering the candidate 154779_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154779_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154824_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154824_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154843_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154843_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154856_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
Preparing report for the candidate 154856_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
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Considering the candidate 154876_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
Preparing report for the candidate 154876_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
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Considering the candidate 154882_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154882_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154894_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154894_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 07:51:28.73 -32:46:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154901_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154901_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154902_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154902_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154926_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154926_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154982_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154982_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154983_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154983_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154990_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154990_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 154998_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 154998_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 155010_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155010_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 155016_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155016_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 155041_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155041_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155048_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155048_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155064_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155064_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155073_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155073_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 155090_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155090_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 155092_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155092_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 155094_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155094_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
Rejecting candidate due to large distance (27.2") between the two second-epoch detections
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Considering the candidate 155096_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155096_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155107_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155107_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 155114_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155114_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 155124_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155124_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 155143_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
Preparing report for the candidate 155143_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
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Considering the candidate 155179_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155179_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 155180_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 155180_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
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Considering the candidate 35555_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 35555_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:04:27.24 -35:15:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33734_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 33734_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:23:19.20 -35:24:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13072_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 13072_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:08:56.55 -37:28:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91172_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 91172_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks
**** FOUND 08:26:04.25 -30:06:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23909_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511
The candidate 23909_fd_Pup-04-Q2b1x1_2026-11-03_03-46-04_20.00sec_0.00C_LIGHT_0511 did not pass the final checks