This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC
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 05 16.4007 2461176.9007 13.38 22:26:42.13 +00:58:53.1
65.92410 -45.26884 galactic Aqr Second-epoch detections are separated by 0.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.690 Wratislavia 0 -1 1 13.6 -0 -0
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:26:42.13 +00:58:53.1: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:26:42.13 +00:58:53.1: 15.83 +/- 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,2461176.9007,13.38,0.05,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 20260516.4007 13.38CV 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 05 16.4007 2461176.9007 13.98 21:53:25.29 +08:33:27.7
66.15698 -34.04335 galactic Peg Second-epoch detections are separated by 0.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.225 Henrietta 0 -0 0 13.8 -0 0
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 21:53:25.29 +08:33:27.7: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 21:53:25.29 +08:33:27.7: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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,2461176.9007,13.98,0.05,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 20260516.4007 13.98CV 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 05 16.4007 2461176.9007 13.18 22:00:33.11 +01:07:27.4
60.38456 -40.14811 galactic Aqr Second-epoch detections are separated by 0.8" and 5.3 pix
The object was found in VSX 1" FASTT 1492
Type: RRAB
# Max. Min./Amp. JD0 Period
13.862 CV Y 1.030 CV 2455086.74030 0.473870000000
The object was not found in astcheck.
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:00:33.11 +01:07:27.4: 14.18 +/- 0.09 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:00:33.11 +01:07:27.4: 14.28 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FASTT 1492,2461176.9007,13.18,0.05,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
FASTT 1492 20260516.4007 13.18CV 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: 2461032.57243787 23.12.2025 01:44:08.632 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
First image: 2461032.57243787 23.12.2025 01:44:08.632 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
Last image: 2461176.90089949 16.05.2026 09:37:07.716 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
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: 16 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): 8818
Objects passed selection criteria: 8813
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: 8207.5
Average stars matched: 8008.5 (97.5754 %)
Memory usage VmPeak: 114356 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat May 16 05:21:53 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: 2461032.57243787 23.12.2025 01:44:08.632 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
First image: 2461032.57243787 23.12.2025 01:44:08.632 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
Last image: 2461176.90089949 16.05.2026 09:37:07.716 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
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: 103 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): 53255
Objects passed selection criteria: 53153
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 46449.8
Average stars matched: 45078.5 (97.0479 %)
Memory usage VmPeak: 153452 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat May 16 05:26:44 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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
SExtractor catalog cache: saved Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat to cache
SExtractor catalog cache: saved Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.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-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.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: 2461176.90044443
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-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits exists and is non-empty
Saving wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits to local_wcs_cache/
'wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits' -> 'local_wcs_cache/wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits'
wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits exists and is non-empty
Saving wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits to local_wcs_cache/
'wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits' -> 'local_wcs_cache/wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits'
wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits exists and is non-empty
Saving wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits to local_wcs_cache/
'wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits' -> 'local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits'
wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits exists and is non-empty
Saving wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits to local_wcs_cache/
'wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits' -> 'local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits (1st reference image)
verification OK: wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.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: 22:17:06.939 +05:59:08.66 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-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits (1st new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
Image size: 941.6'x626.7' 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: 22:17:12.642 +05:58:21.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:06.939 +05:59:08.66
Second-epoch image center 22:17:12.642 +05:58:21.60
Angular distance between the image centers 0.0270 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits (2nd new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
Image size: 941.6'x626.7' 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: 22:17:10.751 +05:58:10.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:06.939 +05:59:08.66
Second-epoch image center 22:17:10.751 +05:58:10.12
Angular distance between the image centers 0.0227 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 22:17:12.642 +05:58:21.60
Second-epoch second image center 22:17:10.751 +05:58:10.12
Angular distance between the image centers 0.00846 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits &> /tmp/tmp.2JOUTNG5yT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits &> /tmp/tmp.R5eackhDT8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits &> /tmp/tmp.qrD2tQlsp9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits &> /tmp/tmp.ICI1h50tA4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.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-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits and wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat
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-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits and wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat
Found non-empty wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits and wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat
The reference image (wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits) and catalog (wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat) found
'wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat' -> 'wcsmag.cat'
Read 9039 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2983 to 342.2677 deg, Dec +0.6997 to +11.2718 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 326.2983 to 342.2677 deg, Dec 0.6997 to 11.2718 deg
Loaded 6082 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): 4963 out of 5222 total matches.
Matched with Tycho-2 5222 out of 9039 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.926500
a=0.000000 b=1.000000 c=22.926500
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.19
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9039 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2983 to 342.2677 deg, Dec +0.6997 to +11.2718 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 326.2983 to 342.2677 deg, Dec 0.6997 to 11.2718 deg
Loaded 6082 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): 4963 out of 5222 total matches.
Matched with Tycho-2 5222 out of 9039 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits:
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits (aperture=6.1)
Read 9065 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2982 to 342.2471 deg, Dec +0.7033 to +11.2727 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 326.2982 to 342.2471 deg, Dec 0.7033 to 11.2727 deg
Loaded 6069 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): 4945 out of 5207 total matches.
Matched with Tycho-2 5207 out of 9065 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits:
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
2.1 pix Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
3.3 pix fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
3.3 pix fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
2.1 pix wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
2.1 pix wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
Limiting magnitude estimates:
15.2 mag. Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
15.2 mag. Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
14.5 mag. fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
14.5 mag. fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2JOUTNG5yT (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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits' -> 'wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=628, passed=9038
Got 9038 stars (including 8398 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 9038 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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 8843 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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 8840 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 8840 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 919 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits N_match=919 sigma_overall_arcsec=0.371 sigma_q1_arcsec=0.463 sigma_q2_arcsec=0.333 sigma_q3_arcsec=0.333 sigma_q4_arcsec=0.367 n_q1=208 n_q2=268 n_q3=179 n_q4=264 worst_quadrant_to_overall_ratio=1.247
The image catalog is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits -region wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.R5eackhDT8 (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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.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-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits' -> 'wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=624, passed=9065
Got 9065 stars (including 8432 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat
util/solve_plate_with_UCAC5 got 9065 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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 8834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 8831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 8831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits N_match=925 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.326 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.340 n_q1=205 n_q2=276 n_q3=179 n_q4=265 worst_quadrant_to_overall_ratio=1.208
The image catalog is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits -region wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qrD2tQlsp9 (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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=313, passed=7458
Got 7458 stars (including 7141 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat
util/solve_plate_with_UCAC5 got 7458 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 7319 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
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 7319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 7319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits N_match=914 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.261 sigma_q4_arcsec=0.341 n_q1=266 n_q2=173 n_q3=275 n_q4=200 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits -region wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ICI1h50tA4 (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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=313, passed=7467
Got 7467 stars (including 7151 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat
util/solve_plate_with_UCAC5 got 7467 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 7325 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
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 7324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 7324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits N_match=911 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.312 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.262 sigma_q4_arcsec=0.300 n_q1=261 n_q2=172 n_q3=279 n_q4=199 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits -region wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits sigma_overall=0.371 worst_q_ratio=1.247
ref2=Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits sigma_overall=0.360 worst_q_ratio=1.208
new1=fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits sigma_overall=0.320 worst_q_ratio=1.241
new2=fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits sigma_overall=0.310 worst_q_ratio=1.146
reference average sigma_overall=0.3655 worst_q_ratio=1.2275
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000_astrometric_residuals.png (919 matched stars from wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001_astrometric_residuals.png (925 matched stars from wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332_astrometric_residuals.png (914 matched stars from wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333_astrometric_residuals.png (911 matched stars from wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits'
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits'
Preparing the HTML report for the field Peg-11-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:03:39.16 +07:21:16.4: 12.36 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:37:03.79 +00:43:25.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:03:39.16 +07:21:16.4: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter REJECTED candidate at 22:03:39.16 +07:21:16.4: ref_mag=12.38 +/- 0.01 new_mean_mag=12.2830 delta=0.10 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:37:03.79 +00:43:25.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:37:03.79 +00:43:25.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
make_report_in_HTML.sh Phase 1 (network queries): 3s
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 20584_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 20584_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
**** FOUND 22:16:03.29 +08:32:52.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20638_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 20638_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
**** FOUND 22:02:40.46 +02:24:15.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20697_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 20697_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20749_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 20749_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04664_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 04664_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
**** FOUND 22:01:02.61 +06:07:10.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Peg-11-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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
SExtractor catalog cache: saved Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat to cache
SExtractor catalog cache: saved Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.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-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
Creating symlink local_wcs_cache/wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.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-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits exists and is non-empty
wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits exists and is non-empty
wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits exists and is non-empty
wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits (1st reference image)
verification OK: wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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: 22:17:06.939 +05:59:08.66 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-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits (1st new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
Image size: 941.6'x626.7' 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: 22:17:12.642 +05:58:21.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:06.939 +05:59:08.66
Second-epoch image center 22:17:12.642 +05:58:21.60
Angular distance between the image centers 0.0270 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits (2nd new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
Image size: 941.6'x626.7' 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: 22:17:10.751 +05:58:10.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:06.939 +05:59:08.66
Second-epoch image center 22:17:10.751 +05:58:10.12
Angular distance between the image centers 0.0227 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 22:17:12.642 +05:58:21.60
Second-epoch second image center 22:17:10.751 +05:58:10.12
Angular distance between the image centers 0.00846 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits &> /tmp/tmp.nSxDnr15eJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits &> /tmp/tmp.wNLPdH9Gu8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits &> /tmp/tmp.qvzFY1UBx4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits &> /tmp/tmp.XuCZRX5pcc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.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-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits and wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat
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-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits and wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat
Found non-empty wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits and wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat
The reference image (wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits) and catalog (wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat) found
'wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat' -> 'wcsmag.cat'
Read 56716 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2894 to 342.2676 deg, Dec +0.6988 to +11.2738 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 326.2894 to 342.2676 deg, Dec 0.6988 to 11.2738 deg
Loaded 6087 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): 4716 out of 5382 total matches.
Matched with Tycho-2 5382 out of 56716 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.801800
a=0.000000 b=1.000000 c=22.801800
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 56716 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2894 to 342.2676 deg, Dec +0.6988 to +11.2738 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 326.2894 to 342.2676 deg, Dec 0.6988 to 11.2738 deg
Loaded 6087 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): 4716 out of 5382 total matches.
Matched with Tycho-2 5382 out of 56716 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits:
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits (aperture=4.7)
Read 56413 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2744 to 342.2604 deg, Dec +0.7027 to +11.2780 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 326.2744 to 342.2604 deg, Dec 0.7027 to 11.2780 deg
Loaded 6094 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): 4728 out of 5377 total matches.
Matched with Tycho-2 5377 out of 56413 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits:
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
2.0 pix Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
3.1 pix fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
3.1 pix fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
2.0 pix wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
2.0 pix wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
Limiting magnitude estimates:
15.3 mag. Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
15.3 mag. Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
14.7 mag. fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
14.7 mag. fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.nSxDnr15eJ (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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits' -> 'wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat corresponding to the image wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=2943, passed=56702
Got 56702 stars (including 53651 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 56702 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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 55609 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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 55607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 55607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 918 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits N_match=918 sigma_overall_arcsec=0.366 sigma_q1_arcsec=0.457 sigma_q2_arcsec=0.330 sigma_q3_arcsec=0.292 sigma_q4_arcsec=0.364 n_q1=207 n_q2=267 n_q3=182 n_q4=262 worst_quadrant_to_overall_ratio=1.247
The image catalog is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits -region wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.wNLPdH9Gu8 (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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.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-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits' -> 'wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat
SExtractor catalog parsing summary: zero_flux=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=2875, passed=56390
Got 56390 stars (including 53403 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat
util/solve_plate_with_UCAC5 got 56390 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
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 55011 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 55010 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 55010 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 917 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits N_match=917 sigma_overall_arcsec=0.371 sigma_q1_arcsec=0.468 sigma_q2_arcsec=0.334 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.344 n_q1=207 n_q2=263 n_q3=178 n_q4=269 worst_quadrant_to_overall_ratio=1.261
The image catalog is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits -region wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qvzFY1UBx4 (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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1508, passed=37047
Got 37047 stars (including 35494 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat
util/solve_plate_with_UCAC5 got 37047 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 904 matched stars entering correct_measured_positions(), 890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 904 matched stars entering correct_measured_positions(), 36352 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 904 matched stars entering correct_measured_positions(), 36354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 904 matched stars entering correct_measured_positions(), 36354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 904 stars left (next iteration limit 994)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits N_match=904 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.394 sigma_q3_arcsec=0.244 sigma_q4_arcsec=0.326 n_q1=256 n_q2=171 n_q3=279 n_q4=198 worst_quadrant_to_overall_ratio=1.225
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits -region wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.XuCZRX5pcc (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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1494, passed=36983
Got 36983 stars (including 35434 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat
util/solve_plate_with_UCAC5 got 36983 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 36242 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
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 36242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 36242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 903 stars left (next iteration limit 993)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits N_match=903 sigma_overall_arcsec=0.312 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.348 sigma_q3_arcsec=0.274 sigma_q4_arcsec=0.323 n_q1=255 n_q2=171 n_q3=282 n_q4=195 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits -region wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-36-28_20.00sec_0.00C_LIGHTs_0332.fits
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.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_2026-05-16_CI_Peg-11-Q1b1x1_051534_TTUQ1b1x1_3874209_4Cv7VveC/wcs_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333.fits
Preparing the HTML report for the field Peg-11-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 21:46:27.93 +01:23:52.4: 13.28 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 21:57:49.03 +10:08:48.2: 12.64 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:37:03.78 +00:43:25.8: 99.00 +/- 99.00 edge
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 21:54:04.89 +05:26:23.4: 13.20 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 21:51:16.31 +05:44:59.6: 11.67 +/- 0.01 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 21:46:27.93 +01:23:52.4: 13.35 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:02:44.62 +08:29:45.1: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:05:55.09 +08:13:19.4: 13.50 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 21:46:27.93 +01:23:52.4: ref_mag=13.31 +/- 0.03 new_mean_mag=13.2827 delta=0.03 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 21:50:34.35 +10:56:02.3: 13.58 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 21:57:49.03 +10:08:48.2: 12.61 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:37:03.78 +00:43:25.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 22:37:03.78 +00:43:25.8: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:14:42.15 +04:15:58.6: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 21:54:04.89 +05:26:23.4: 13.24 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 21:57:49.03 +10:08:48.2: ref_mag=12.62 +/- 0.02 new_mean_mag=12.6300 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 21:51:16.31 +05:44:59.6: 11.60 +/- 0.01 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:02:44.62 +08:29:45.1: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter REJECTED candidate at 21:54:04.89 +05:26:23.4: ref_mag=13.22 +/- 0.02 new_mean_mag=13.1858 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:02:44.62 +08:29:45.1: ref_mag=13.22 +/- 0.02 new_mean_mag=13.1246 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:51:16.31 +05:44:59.6: ref_mag=11.64 +/- 0.01 new_mean_mag=11.9067 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 21:54:18.11 +04:18:46.7: 13.61 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:05:55.09 +08:13:19.4: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter REJECTED candidate at 22:05:55.09 +08:13:19.4: ref_mag=13.49 +/- 0.03 new_mean_mag=13.4241 delta=0.06 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 21:50:34.35 +10:56:02.3: 13.57 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Forced photometry filter REJECTED candidate at 21:50:34.35 +10:56:02.3: ref_mag=13.58 +/- 0.04 new_mean_mag=13.5528 delta=0.03 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:14:42.15 +04:15:58.6: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter REJECTED candidate at 22:14:42.15 +04:15:58.6: ref_mag=13.42 +/- 0.03 new_mean_mag=13.2131 delta=0.21 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 21:54:18.11 +04:18:46.7: 13.50 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter REJECTED candidate at 21:54:18.11 +04:18:46.7: ref_mag=13.55 +/- 0.03 new_mean_mag=13.4597 delta=0.09 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:17:22.07 +08:11:27.0: 13.79 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 21:52:44.47 +06:52:50.0: 13.96 +/- 0.07 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:26:42.13 +00:58:53.1: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 21:53:25.29 +08:33:27.7: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:15:31.25 +01:55:47.9: 13.34 +/- 0.04 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:08:51.74 +03:04:35.7: 13.74 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 21:52:44.47 +06:52:50.0: 14.07 +/- 0.07 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:06:43.19 +11:05:45.7: 15.07 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Forced photometry filter REJECTED candidate at 21:52:44.47 +06:52:50.0: ref_mag=14.01 +/- 0.05 new_mean_mag=13.8245 delta=0.19 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 21:53:06.99 +09:13:53.8: 14.85 +/- 0.16 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:15:31.25 +01:55:47.9: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter REJECTED candidate at 22:15:31.25 +01:55:47.9: ref_mag=13.30 +/- 0.03 new_mean_mag=13.3443 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 21:53:25.29 +08:33:27.7: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:26:42.13 +00:58:53.1: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:08:51.74 +03:04:35.7: 13.75 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:02:00.43 +05:36:52.6: 15.57 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter REJECTED candidate at 22:08:51.74 +03:04:35.7: ref_mag=13.75 +/- 0.04 new_mean_mag=13.7409 delta=0.01 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:17:22.07 +08:11:27.0: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter REJECTED candidate at 22:17:22.07 +08:11:27.0: ref_mag=13.75 +/- 0.04 new_mean_mag=13.7048 delta=0.05 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:06:43.19 +11:05:45.7: 14.84 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.11
Forced photometry filter REJECTED candidate at 22:06:43.19 +11:05:45.7: ref_mag=14.93 +/- 0.11 new_mean_mag=14.7521 delta=0.18 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 21:53:06.99 +09:13:53.8: 14.79 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.11
Forced photometry filter REJECTED candidate at 21:53:06.99 +09:13:53.8: ref_mag=14.82 +/- 0.11 new_mean_mag=14.5357 delta=0.28 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:02:00.43 +05:36:52.6: 15.13 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.14
Forced photometry filter REJECTED candidate at 22:02:00.43 +05:36:52.6: ref_mag=15.26 +/- 0.14 new_mean_mag=14.5510 delta=0.71 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-08_20.00sec_-15.00C_LIGHT_0000.fits at 22:00:33.11 +01:07:27.4: 14.18 +/- 0.09 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2025-12-22_19-44-47_20.00sec_-15.00C_LIGHT_0001.fits at 22:00:33.11 +01:07:27.4: 14.28 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.06
Forced photometry filter KEPT candidate at 22:00:33.11 +01:07:27.4: ref_mag=14.23 +/- 0.06 new_mean_mag=13.1826 delta=1.04 (need > 0.90)
Adding exclusion_list_local.txt__out37598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71601.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
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: 5s
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Considering the candidate 70787_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 70787_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 70790_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 70790_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 70791_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 70791_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 70794_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 70794_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 70850_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 70850_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
**** FOUND 22:16:03.29 +08:32:52.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 70968_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 70968_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 70984_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 70984_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
**** FOUND 22:15:16.70 +01:40:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71026_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71026_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
**** FOUND 22:19:34.62 +09:06:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71056_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71056_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71245_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71245_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
**** FOUND 22:35:35.01 +10:20:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71322_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71322_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71340_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71340_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71341_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71341_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71364_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71364_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71399_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71399_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71459_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
Preparing report for the candidate 71459_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
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Considering the candidate 71514_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71514_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71516_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71516_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71568_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71568_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71601_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
Preparing report for the candidate 71601_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
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Considering the candidate 71861_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71861_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71882_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71882_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 71900_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 71900_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
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Considering the candidate 44136_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 44136_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks
**** FOUND 22:02:40.46 +02:24:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37598_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
Preparing report for the candidate 37598_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
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Considering the candidate 29193_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333
The candidate 29193_fd_Peg-11-Q1b1x1_2026-05-16_04-37-07_20.00sec_-0.00C_LIGHTs_0333 did not pass the final checks