This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6
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 07 27.3848 2461248.8848 12.40 00:09:57.24 +20:01:19.4
109.81977 -41.79107 galactic Peg Second-epoch detections are separated by 0.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.71 Niobe -0 -1 1 12.5 0 0
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:09:57.24 +20:01:19.4: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:09:57.24 +20:01:19.4: 16.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.8848,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.3848 12.40CV 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 07 27.3848 2461248.8848 12.62 00:07:27.56 +20:38:40.8
109.24164 -41.05506 galactic Peg Second-epoch detections are separated by 0.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.695 Bella -1 -1 1 12.9 -0 0
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:07:27.56 +20:38:40.8: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:07:27.56 +20:38:40.8: 16.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.8848,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.3848 12.62CV 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 07 27.3848 2461248.8848 13.95 00:10:02.51 +16:57:12.8
108.91998 -44.78899 galactic Peg Second-epoch detections are separated by 1.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.665 Sabine 1 -0 1 14.0 -0 -0
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:10:02.51 +16:57:12.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:10:02.51 +16:57:12.8: 15.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.8848,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.3848 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.3848 2461248.8848 14.67 23:40:05.88 +18:27:55.7
100.20632 -41.23684 galactic Peg Second-epoch detections are separated by 2.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.879 Ricarda -1 -1 2 14.8 -0 -0
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:40:05.88 +18:27:55.7: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:40:05.88 +18:27:55.7: 15.92 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.8848,14.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.3848 14.67CV 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: 2461049.62147831 09.01.2026 02:54:45.726 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
First image: 2461049.62147831 09.01.2026 02:54:45.726 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Last image: 2461248.88510038 27.07.2026 09:14:22.673 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 95 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8888
Objects passed selection criteria: 8884
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 8390.75
Average stars matched: 8216.25 (97.9203 %)
Memory usage VmPeak: 234688 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 27 04:47:39 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.62147831 09.01.2026 02:54:45.726 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
First image: 2461049.62147831 09.01.2026 02:54:45.726 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Last image: 2461248.88510038 27.07.2026 09:14:22.673 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 36
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 35 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 51745
Objects passed selection criteria: 51623
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: 47923.8
Average stars matched: 46727.5 (97.5038 %)
Memory usage VmPeak: 272156 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 27 04:52:44 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
SExtractor catalog cache: saved Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.cat to cache
SExtractor catalog cache: saved Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.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/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461248.88444486
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
Saving wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits to local_wcs_cache/
'wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits' -> 'local_wcs_cache/wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits'
wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits exists and is non-empty
Saving wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits to local_wcs_cache/
'wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits' -> 'local_wcs_cache/wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits'
wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits exists and is non-empty
Saving wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits to local_wcs_cache/
'wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits' -> 'local_wcs_cache/wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits'
wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits exists and is non-empty
Saving wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits to local_wcs_cache/
'wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits' -> 'local_wcs_cache/wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits (1st reference image)
verification OK: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:00.348 +21:59:54.97 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits (1st new image)
verification OK: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:59.948 +22:00:09.50 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.348 +21:59:54.97
Second-epoch image center 23:59:59.948 +22:00:09.50
Angular distance between the image centers 0.0043 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits (2nd new image)
verification OK: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:02.866 +22:00:08.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.348 +21:59:54.97
Second-epoch image center 00:00:02.866 +22:00:08.39
Angular distance between the image centers 0.0104 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 23:59:59.948 +22:00:09.50
Second-epoch second image center 00:00:02.866 +22:00:08.39
Angular distance between the image centers 0.01128 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/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.XcFKIi79jK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits &> /tmp/tmp.E3btwzum6f
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits &> /tmp/tmp.RwIGuuuOq6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits &> /tmp/tmp.e6waK97GrJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
Found non-empty wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
The reference image (wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits) and catalog (wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat) found
'wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 9019 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2902 to 8.8792 deg, Dec +16.5101 to +27.2962 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 351.2902 to 8.8792 deg, Dec 16.5101 to 27.2962 deg
Loaded 6920 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): 5313 out of 5630 total matches.
Matched with Tycho-2 5630 out of 9019 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881100
a=0.000000 b=1.000000 c=22.881100
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.27
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.27
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 9019 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2902 to 8.8792 deg, Dec +16.5101 to +27.2962 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 351.2902 to 8.8792 deg, Dec 16.5101 to 27.2962 deg
Loaded 6920 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): 5313 out of 5630 total matches.
Matched with Tycho-2 5630 out of 9019 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits:
Forced-photometry filter: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits -> calib.txt_param_ref_wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits (aperture=5.9)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 8998 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2893 to 8.8790 deg, Dec +16.5101 to +27.2944 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 351.2893 to 8.8790 deg, Dec 16.5101 to 27.2944 deg
Loaded 6921 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): 5335 out of 5642 total matches.
Matched with Tycho-2 5642 out of 8998 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits:
Forced-photometry filter: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits -> calib.txt_param_ref_wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
2.0 pix Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
2.6 pix fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
2.6 pix fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
2.0 pix wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
2.0 pix wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Limiting magnitude estimates:
15.3 mag. Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
15.3 mag. Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
14.9 mag. fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
14.9 mag. fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.XcFKIi79jK (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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits' -> 'wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=673, bad_region=0, passed=9019
Got 9019 stars (including 8339 good ones) from the SExtractor catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
util/solve_plate_with_UCAC5 got 9019 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2902 through 0 to 8.8792, gap 8.8792 to 351.2902
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 8856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2904 through 0 to 8.8801, gap 8.8801 to 351.2904
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 8856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 8856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits N_match=971 sigma_overall_arcsec=0.323 sigma_q1_arcsec=0.406 sigma_q2_arcsec=0.341 sigma_q3_arcsec=0.324 sigma_q4_arcsec=0.270 n_q1=235 n_q2=245 n_q3=227 n_q4=264 worst_quadrant_to_overall_ratio=1.257
The image catalog is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.E3btwzum6f (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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits' -> 'wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.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/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Checking if the catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS catalog name: wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=657, bad_region=0, passed=8998
Got 8998 stars (including 8327 good ones) from the SExtractor catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat
util/solve_plate_with_UCAC5 got 8998 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2893 through 0 to 8.8790, gap 8.8790 to 351.2893
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 8864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2888 through 0 to 8.8799, gap 8.8799 to 351.2888
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 8862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 8862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits N_match=971 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.356 sigma_q2_arcsec=0.307 sigma_q3_arcsec=0.264 sigma_q4_arcsec=0.263 n_q1=238 n_q2=245 n_q3=227 n_q4=261 worst_quadrant_to_overall_ratio=1.181
The image catalog is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits -region wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.RwIGuuuOq6 (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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
Checking if the catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
WCS catalog name: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=397, bad_region=0, passed=7855
Got 7855 stars (including 7448 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 7855 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.4858 through 0 to 9.0762, gap 9.0762 to 351.4858
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 7753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.4855 through 0 to 9.0768, gap 9.0768 to 351.4855
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 7752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 7752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=977 robust_rms=10.640 arcsec
SIP_REFIT: SIP order 3 trial: matched=977 robust_rms=0.337 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=977 robust_rms_before=0.878 arcsec robust_rms_before_corrected=0.300 arcsec robust_rms_after=0.337 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.300 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits N_match=977 sigma_overall_arcsec=0.290 sigma_q1_arcsec=0.256 sigma_q2_arcsec=0.353 sigma_q3_arcsec=0.279 sigma_q4_arcsec=0.259 n_q1=242 n_q2=239 n_q3=241 n_q4=255 worst_quadrant_to_overall_ratio=1.216
The image catalog is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits -region wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.e6waK97GrJ (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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
Checking if the catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
WCS catalog name: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=405, bad_region=0, passed=7871
Got 7871 stars (including 7457 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat
util/solve_plate_with_UCAC5 got 7871 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.4990 through 0 to 9.0763, gap 9.0763 to 351.4990
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 7771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.4989 through 0 to 9.0769, gap 9.0769 to 351.4989
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 7770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 7770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=977 robust_rms=10.703 arcsec
SIP_REFIT: SIP order 3 trial: matched=977 robust_rms=0.346 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=977 robust_rms_before=0.888 arcsec robust_rms_before_corrected=0.303 arcsec robust_rms_after=0.346 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.303 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits N_match=977 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.281 n_q1=244 n_q2=232 n_q3=243 n_q4=258 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits -region wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits sigma_overall=0.323 worst_q_ratio=1.257
ref2=Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits sigma_overall=0.302 worst_q_ratio=1.181
new1=fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits sigma_overall=0.290 worst_q_ratio=1.216
new2=fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits sigma_overall=0.304 worst_q_ratio=1.116
reference average sigma_overall=0.3125 worst_q_ratio=1.219
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067_astrometric_residuals.png (971 matched stars from wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068_astrometric_residuals.png (971 matched stars from wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258_astrometric_residuals.png (977 matched stars from wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259_astrometric_residuals.png (977 matched stars from wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits'
Saving fully-calibrated image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits'
Preparing the HTML report for the field Peg-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:07:55.72 +21:19:24.5: 12.30 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:52:14.56 +19:10:35.8: 12.22 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:43:54.87 +21:58:27.6: 12.20 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:58:11.07 +22:35:12.1: 12.29 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:45:18.47 +21:02:37.7: 12.34 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:10:33.47 +21:44:47.5: 12.21 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:05:02.12 +22:26:01.2: 12.18 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:58:31.76 +20:34:23.2: 12.38 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:11:33.29 +21:27:27.8: 12.20 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:07:55.72 +21:19:24.5: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter REJECTED candidate at 00:07:55.72 +21:19:24.5: ref_mag=12.32 +/- 0.01 new_mean_mag=12.2831 delta=0.03 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:10:33.47 +21:44:47.5: 12.24 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:52:14.56 +19:10:35.8: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter REJECTED candidate at 23:52:14.56 +19:10:35.8: ref_mag=12.23 +/- 0.01 new_mean_mag=12.1631 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:10:33.47 +21:44:47.5: ref_mag=12.23 +/- 0.01 new_mean_mag=12.2139 delta=0.01 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:43:54.87 +21:58:27.6: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter REJECTED candidate at 23:43:54.87 +21:58:27.6: ref_mag=12.23 +/- 0.01 new_mean_mag=12.1584 delta=0.07 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:58:11.07 +22:35:12.1: 12.26 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:11:33.29 +21:27:27.8: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Forced photometry filter REJECTED candidate at 23:58:11.07 +22:35:12.1: ref_mag=12.27 +/- 0.01 new_mean_mag=12.2163 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter REJECTED candidate at 00:11:33.29 +21:27:27.8: ref_mag=12.19 +/- 0.01 new_mean_mag=12.2948 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:45:18.47 +21:02:37.7: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter REJECTED candidate at 23:45:18.47 +21:02:37.7: ref_mag=12.33 +/- 0.01 new_mean_mag=12.2979 delta=0.04 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:05:02.12 +22:26:01.2: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 00:05:02.12 +22:26:01.2: ref_mag=12.17 +/- 0.01 new_mean_mag=12.1269 delta=0.04 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:58:31.76 +20:34:23.2: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter REJECTED candidate at 23:58:31.76 +20:34:23.2: ref_mag=12.37 +/- 0.01 new_mean_mag=12.3171 delta=0.05 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20439_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 20439_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20571_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 20571_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20576_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 20576_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20578_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 20578_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20583_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 20583_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20584_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 20584_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20587_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 20587_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20591_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 20591_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20598_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 20598_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00820_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 00820_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 00:32:22.41 +26:01:44.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Peg-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
SExtractor catalog cache: saved Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.cat to cache
SExtractor catalog cache: saved Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Creating symlink local_wcs_cache/wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits exists and is non-empty
wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits exists and is non-empty
wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits (1st reference image)
verification OK: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:00.348 +21:59:54.97 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits (1st new image)
verification OK: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:59.948 +22:00:09.50 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.348 +21:59:54.97
Second-epoch image center 23:59:59.948 +22:00:09.50
Angular distance between the image centers 0.0043 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits (2nd new image)
verification OK: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:02.866 +22:00:08.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.348 +21:59:54.97
Second-epoch image center 00:00:02.866 +22:00:08.39
Angular distance between the image centers 0.0104 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 23:59:59.948 +22:00:09.50
Second-epoch second image center 00:00:02.866 +22:00:08.39
Angular distance between the image centers 0.01128 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/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.06pFCLHukO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits &> /tmp/tmp.VbqgCDNReM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits &> /tmp/tmp.JgrxoH1XCF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits &> /tmp/tmp.bPPwoYg4gY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
Found non-empty wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
The reference image (wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits) and catalog (wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat) found
'wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 54563 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2893 to 8.8872 deg, Dec +16.4838 to +27.3003 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 351.2893 to 8.8872 deg, Dec 16.4838 to 27.3003 deg
Loaded 6940 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): 5095 out of 5798 total matches.
Matched with Tycho-2 5798 out of 54563 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.777100
a=0.000000 b=1.000000 c=22.777100
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 54563 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2893 to 8.8872 deg, Dec +16.4838 to +27.3003 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 351.2893 to 8.8872 deg, Dec 16.4838 to 27.3003 deg
Loaded 6940 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): 5095 out of 5798 total matches.
Matched with Tycho-2 5798 out of 54563 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits:
Forced-photometry filter: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits -> calib.txt_param_ref_wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits (aperture=4.7)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 54021 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2769 to 8.8790 deg, Dec +16.4843 to +27.2989 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 351.2769 to 8.8790 deg, Dec 16.4843 to 27.2989 deg
Loaded 6948 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): 5113 out of 5797 total matches.
Matched with Tycho-2 5797 out of 54021 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits:
Forced-photometry filter: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits -> calib.txt_param_ref_wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
1.9 pix Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
2.5 pix fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
2.5 pix fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
1.9 pix wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
1.9 pix wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Limiting magnitude estimates:
15.4 mag. Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
15.4 mag. Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
15.0 mag. fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
15.0 mag. fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (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.06pFCLHukO (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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits' -> 'wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=2723, bad_region=3, passed=54549
Got 54549 stars (including 51710 good ones) from the SExtractor catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
util/solve_plate_with_UCAC5 got 54549 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2893 through 0 to 8.8872, gap 8.8872 to 351.2893
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 53722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2889 through 0 to 8.8880, gap 8.8880 to 351.2889
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 53722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 53721 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits N_match=971 sigma_overall_arcsec=0.332 sigma_q1_arcsec=0.397 sigma_q2_arcsec=0.298 sigma_q3_arcsec=0.323 sigma_q4_arcsec=0.290 n_q1=231 n_q2=242 n_q3=227 n_q4=271 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VbqgCDNReM (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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits' -> 'wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.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/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Checking if the catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS catalog name: wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2675, bad_region=3, passed=54003
Got 54003 stars (including 51231 good ones) from the SExtractor catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat
util/solve_plate_with_UCAC5 got 54003 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2769 through 0 to 8.8790, gap 8.8790 to 351.2769
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 53084 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2765 through 0 to 8.8799, gap 8.8799 to 351.2765
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 53085 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 53085 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits N_match=971 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.349 sigma_q2_arcsec=0.296 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.256 n_q1=230 n_q2=236 n_q3=234 n_q4=271 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits -region wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JgrxoH1XCF (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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
Checking if the catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
WCS catalog name: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1614, bad_region=5, passed=42059
Got 42059 stars (including 40365 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 42059 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.4858 through 0 to 9.0761, gap 9.0761 to 351.4858
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 41815 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.4855 through 0 to 9.0768, gap 9.0768 to 351.4855
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 41817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 41817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits N_match=977 sigma_overall_arcsec=0.296 sigma_q1_arcsec=0.287 sigma_q2_arcsec=0.306 sigma_q3_arcsec=0.270 sigma_q4_arcsec=0.277 n_q1=243 n_q2=240 n_q3=242 n_q4=252 worst_quadrant_to_overall_ratio=1.035
The image catalog is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits -region wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bPPwoYg4gY (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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
Checking if the catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
WCS catalog name: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1641, bad_region=12, passed=42246
Got 42246 stars (including 40524 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat
util/solve_plate_with_UCAC5 got 42246 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.4977 through 0 to 9.0763, gap 9.0763 to 351.4977
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 41870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.4974 through 0 to 9.0768, gap 9.0768 to 351.4974
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 41870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 41870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits N_match=977 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.319 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.317 n_q1=241 n_q2=232 n_q3=245 n_q4=259 worst_quadrant_to_overall_ratio=1.017
The image catalog is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits -region wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-13-26_20.00sec_-0.00C_LIGHTs_0258.fits
Saving fully-calibrated image wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.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_2026-07-27_CI_Peg-04-Q1b1x1_041625_TTUQ1b1x1_3628768_Cz917AJ6/wcs_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259.fits
Preparing the HTML report for the field Peg-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:07:27.56 +20:38:40.8: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:09:57.24 +20:01:19.4: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:56:08.28 +20:06:26.7: 13.37 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:44:59.88 +24:06:51.6: 11.16 +/- 0.00 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:33:31.58 +19:43:47.9: 13.72 +/- 0.05 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:44:13.60 +20:38:13.6: 12.59 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:29:55.75 +21:59:47.1: 14.35 +/- 0.10 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:54:55.13 +25:26:50.3: 13.81 +/- 0.05 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:56:08.28 +20:06:26.7: 13.46 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:44:59.88 +24:06:51.6: 11.16 +/- 0.00 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry reference-image weighted average: 11.16 +/- 0.00
Forced photometry filter REJECTED candidate at 23:56:08.28 +20:06:26.7: ref_mag=13.41 +/- 0.02 new_mean_mag=13.5826 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:44:59.88 +24:06:51.6: ref_mag=11.16 +/- 0.00 new_mean_mag=11.3485 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:09:57.24 +20:01:19.4: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:07:27.56 +20:38:40.8: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:44:13.60 +20:38:13.6: 12.58 +/- 0.02 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:29:55.75 +21:59:47.1: 14.41 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter REJECTED candidate at 23:44:13.60 +20:38:13.6: ref_mag=12.58 +/- 0.01 new_mean_mag=12.6004 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 14.38 +/- 0.07
Forced photometry filter REJECTED candidate at 23:29:55.75 +21:59:47.1: ref_mag=14.38 +/- 0.07 new_mean_mag=14.2765 delta=0.10 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:33:31.58 +19:43:47.9: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter REJECTED candidate at 23:33:31.58 +19:43:47.9: ref_mag=13.69 +/- 0.04 new_mean_mag=14.0836 delta=-0.39 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:54:55.13 +25:26:50.3: 13.86 +/- 0.05 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:31:33.69 +20:50:54.9: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Forced photometry filter REJECTED candidate at 23:54:55.13 +25:26:50.3: ref_mag=13.83 +/- 0.03 new_mean_mag=14.0397 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:31:33.69 +20:50:54.9: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter REJECTED candidate at 00:31:33.69 +20:50:54.9: ref_mag=12.66 +/- 0.02 new_mean_mag=12.6451 delta=0.02 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:18:25.19 +26:07:47.4: 13.57 +/- 0.05 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:39:22.62 +24:43:45.6: 13.52 +/- 0.04 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:50:15.20 +23:47:30.1: 13.61 +/- 0.04 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:35:46.19 +20:34:47.3: 13.79 +/- 0.05 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:12:43.84 +26:31:10.8: 13.75 +/- 0.05 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:39:22.62 +24:43:45.6: 13.55 +/- 0.05 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:18:25.19 +26:07:47.4: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Forced photometry filter REJECTED candidate at 00:18:25.19 +26:07:47.4: ref_mag=13.59 +/- 0.04 new_mean_mag=13.5420 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:39:22.62 +24:43:45.6: ref_mag=13.53 +/- 0.03 new_mean_mag=13.3875 delta=0.15 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:59:58.48 +25:52:52.6: 13.33 +/- 0.04 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:50:15.20 +23:47:30.1: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter REJECTED candidate at 23:50:15.20 +23:47:30.1: ref_mag=13.62 +/- 0.03 new_mean_mag=13.6532 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:57:56.41 +25:07:26.6: 13.84 +/- 0.06 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:35:46.19 +20:34:47.3: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:51:36.02 +24:17:54.0: 13.90 +/- 0.05 detection
Forced photometry filter REJECTED candidate at 23:35:46.19 +20:34:47.3: ref_mag=13.78 +/- 0.04 new_mean_mag=13.6459 delta=0.13 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:59:58.48 +25:52:52.6: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter REJECTED candidate at 23:59:58.48 +25:52:52.6: ref_mag=13.29 +/- 0.02 new_mean_mag=13.7431 delta=-0.46 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:57:56.41 +25:07:26.6: 13.72 +/- 0.06 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:12:43.84 +26:31:10.8: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter REJECTED candidate at 23:57:56.41 +25:07:26.6: ref_mag=13.78 +/- 0.04 new_mean_mag=13.8492 delta=-0.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Forced photometry filter REJECTED candidate at 00:12:43.84 +26:31:10.8: ref_mag=13.72 +/- 0.03 new_mean_mag=13.6407 delta=0.08 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:51:36.02 +24:17:54.0: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Forced photometry filter REJECTED candidate at 23:51:36.02 +24:17:54.0: ref_mag=13.89 +/- 0.04 new_mean_mag=13.8973 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:20:47.95 +26:29:29.7: 13.82 +/- 0.06 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:24:00.87 +18:06:48.3: 13.81 +/- 0.06 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:10:02.51 +16:57:12.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:40:34.80 +22:29:32.9: 14.02 +/- 0.07 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:20:47.95 +26:29:29.7: 13.77 +/- 0.06 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:24:00.87 +18:06:48.3: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter REJECTED candidate at 00:20:47.95 +26:29:29.7: ref_mag=13.79 +/- 0.04 new_mean_mag=13.9379 delta=-0.14 (need > 0.90)
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Forced photometry filter REJECTED candidate at 00:24:00.87 +18:06:48.3: ref_mag=13.83 +/- 0.04 new_mean_mag=13.7939 delta=0.04 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:21:55.01 +22:00:21.6: 14.45 +/- 0.09 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:40:34.80 +22:29:32.9: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Forced photometry filter REJECTED candidate at 23:40:34.80 +22:29:32.9: ref_mag=14.02 +/- 0.05 new_mean_mag=14.0709 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:10:02.51 +16:57:12.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:21:55.01 +22:00:21.6: 14.47 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.06
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:48:27.45 +24:56:23.5: 14.47 +/- 0.08 detection
Forced photometry filter REJECTED candidate at 00:21:55.01 +22:00:21.6: ref_mag=14.46 +/- 0.06 new_mean_mag=14.1607 delta=0.30 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:40:05.88 +18:27:55.7: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:36:43.13 +20:09:03.0: 15.27 +/- 0.21 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:48:27.45 +24:56:23.5: 14.53 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.06
Forced photometry filter REJECTED candidate at 23:48:27.45 +24:56:23.5: ref_mag=14.50 +/- 0.06 new_mean_mag=14.6155 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:38:32.62 +27:03:08.0: 15.10 +/- 0.19 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:07:19.87 +22:15:52.2: 14.57 +/- 0.09 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:40:05.88 +18:27:55.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:36:43.13 +20:09:03.0: 15.13 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.14
Forced photometry filter REJECTED candidate at 23:36:43.13 +20:09:03.0: ref_mag=15.19 +/- 0.14 new_mean_mag=14.7066 delta=0.48 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:38:32.62 +27:03:08.0: 15.02 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.13
Forced photometry filter REJECTED candidate at 23:38:32.62 +27:03:08.0: ref_mag=15.06 +/- 0.13 new_mean_mag=14.5977 delta=0.46 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:07:19.87 +22:15:52.2: 14.68 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.07
Forced photometry filter REJECTED candidate at 00:07:19.87 +22:15:52.2: ref_mag=14.62 +/- 0.07 new_mean_mag=14.5634 delta=0.06 (need > 0.90)
Adding exclusion_list_local.txt__out68261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68937.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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: 6s
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Considering the candidate 68072_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68072_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68076_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68076_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68077_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68077_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68080_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68080_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 23:30:40.92 +20:13:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68082_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68082_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68084_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68084_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 23:28:10.80 +25:55:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68086_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68086_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68087_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68087_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68261_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
Preparing report for the candidate 68261_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
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Considering the candidate 68301_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
Preparing report for the candidate 68301_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
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Considering the candidate 68312_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68312_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68341_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68341_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 00:27:28.11 +26:18:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68459_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68459_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68510_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68510_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68529_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68529_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 00:15:01.49 +22:17:41.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 68534_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68534_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68535_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68535_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68548_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68548_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68551_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68551_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68597_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68597_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68634_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68634_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68640_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68640_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68645_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68645_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68654_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68654_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 23:33:30.79 +23:14:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68674_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
Preparing report for the candidate 68674_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
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Considering the candidate 68698_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68698_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68701_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68701_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 23:33:32.15 +24:21:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68733_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68733_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68741_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68741_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 23:43:29.16 +25:06:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68916_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68916_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68924_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68924_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68930_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68930_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 68937_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
Preparing report for the candidate 68937_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
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Considering the candidate 68963_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 68963_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 04721_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259
The candidate 04721_fd_Peg-04-Q1b1x1_2026-07-27_04-14-22_20.00sec_0.00C_LIGHTs_0259 did not pass the final checks