This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT
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 10 07.3689 2461320.8689 13.35 22:52:34.54 +13:40:58.4
83.95767 -40.02736 galactic Peg Second-epoch detections are separated by 0.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.170 Maria 0 -0 0 13.2 -0 -0
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:52:34.54 +13:40:58.4: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:52:34.54 +13:40:58.4: 15.95 +/- 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,2461320.8689,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261007.3689 13.35CV 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 10 07.3689 2461320.8689 14.05 23:23:07.07 +10:47:44.3
90.52844 -46.44482 galactic Peg Second-epoch detections are separated by 1.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1001 Gaussia -0 -0 0 14.1 -0 0
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:23:07.07 +10:47:44.3: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:23:07.07 +10:47:44.3: 15.97 +/- 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,2461320.8689,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261007.3689 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 07.3689 2461320.8689 15.00 23:12:58.08 +17:07:36.4
91.76773 -39.71252 galactic Peg Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.4914 Pardina 1 0 1 14.9 0 0
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:12:58.08 +17:07:36.4: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:12:58.08 +17:07:36.4: 16.02 +/- 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,2461320.8689,15.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261007.3689 15.00CV 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 10 07.3689 2461320.8689 14.93 22:48:39.27 +16:15:55.3
84.86275 -37.36896 galactic Peg Second-epoch detections are separated by 3.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.430 Hybris -1 -1 1 14.7 0 0
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:48:39.27 +16:15:55.3: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:48:39.27 +16:15:55.3: 15.91 +/- 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,2461320.8689,14.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261007.3689 14.93CV 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: 2461242.89976286 21.07.2026 09:35:29.511 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
First image: 2461242.89976286 21.07.2026 09:35:29.511 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Last image: 2461320.86928439 07.10.2026 08:51:36.171 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.16
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 8549
Objects passed selection criteria: 8518
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 6664.5
Average stars matched: 6152 (92.31 %)
Memory usage VmPeak: 233932 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 7 12:08:09 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: 2461242.89976286 21.07.2026 09:35:29.511 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
First image: 2461242.89976286 21.07.2026 09:35:29.511 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Last image: 2461320.86928439 07.10.2026 08:51:36.171 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 42
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.89
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 60 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 50015
Objects passed selection criteria: 49828
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 40426.2
Average stars matched: 36963.2 (91.4338 %)
Memory usage VmPeak: 266316 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 7 12:10:12 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/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.cat to cache
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461320.86846431
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-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits exists and is non-empty
wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits exists and is non-empty
wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits exists and is non-empty
wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (1st reference image)
verification OK: wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:39.243 +14:00:09.40 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:39.416 +14:00:08.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:39.243 +14:00:09.40
Second-epoch image center 23:06:39.416 +14:00:08.23
Angular distance between the image centers 0.0008 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:36.885 +13:59:33.28 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:39.243 +14:00:09.40
Second-epoch image center 23:06:36.885 +13:59:33.28
Angular distance between the image centers 0.0138 deg.
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# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:06:39.416 +14:00:08.23
Second-epoch second image center 23:06:36.885 +13:59:33.28
Angular distance between the image centers 0.01410 deg.
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Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits &> /tmp/tmp.CLvYTNeEy9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits &> /tmp/tmp.EVgzH0PpDE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits &> /tmp/tmp.184VCaUOZm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits &> /tmp/tmp.G3KMJRJiiM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
Found non-empty wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
The reference image (wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits) and catalog (wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat) found
'wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat' -> 'wcsmag.cat'
Read 9326 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4001 to 354.8631 deg, Dec +8.6411 to +19.2659 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 338.4001 to 354.8631 deg, Dec 8.6411 to 19.2659 deg
Loaded 5954 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): 4864 out of 5041 total matches.
Matched with Tycho-2 5041 out of 9326 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.684400
a=0.000000 b=1.000000 c=22.684400
From vast_summary.log: estimated ref. image limiting mag.: -7.16
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9326 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4001 to 354.8631 deg, Dec +8.6411 to +19.2659 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 338.4001 to 354.8631 deg, Dec 8.6411 to 19.2659 deg
Loaded 5954 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): 4864 out of 5041 total matches.
Matched with Tycho-2 5041 out of 9326 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (aperture=6.2)
Read 8960 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4002 to 354.8630 deg, Dec +8.6412 to +19.2650 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 338.4002 to 354.8630 deg, Dec 8.6412 to 19.2650 deg
Loaded 5954 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): 4852 out of 5019 total matches.
Matched with Tycho-2 5019 out of 8960 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
2.2 pix Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
2.4 pix fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
2.3 pix fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Limiting magnitude estimates:
15.5 mag. Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
15.5 mag. Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
15.3 mag. fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
15.3 mag. fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.CLvYTNeEy9 (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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits' -> 'wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=501, bad_region=1909, passed=9326
Got 9326 stars (including 6993 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
util/solve_plate_with_UCAC5 got 9326 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 4853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 7766 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 7766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 7766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4852 stars left (next iteration limit 5338)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits N_match=4852 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.312 sigma_q2_arcsec=0.346 sigma_q3_arcsec=0.405 sigma_q4_arcsec=0.331 n_q1=1495 n_q2=839 n_q3=1685 n_q4=833 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits -region wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.EVgzH0PpDE (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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits' -> 'wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=477, bad_region=1851, passed=8960
Got 8960 stars (including 6707 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat
util/solve_plate_with_UCAC5 got 8960 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 4854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 7457 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 7457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 7457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4854 stars left (next iteration limit 5339)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits N_match=4854 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.320 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.396 sigma_q4_arcsec=0.343 n_q1=1493 n_q2=837 n_q3=1694 n_q4=830 worst_quadrant_to_overall_ratio=1.106
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits -region wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.184VCaUOZm (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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=417, bad_region=2118, passed=8251
Got 8251 stars (including 5803 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat
util/solve_plate_with_UCAC5 got 8251 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 4885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 6563 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 6563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 6563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4885 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4885 robust_rms=7.617 arcsec worst_region_rms=13.988 arcsec outer_annulus_rms=13.988 arcsec
SIP_REFIT: SIP order 3 trial: matched=4885 robust_rms=0.487 arcsec worst_region_rms=1.065 arcsec outer_annulus_rms=1.065 arcsec
SIP_REFIT: SIP order 5 trial: matched=4885 robust_rms=0.357 arcsec worst_region_rms=0.436 arcsec outer_annulus_rms=0.436 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4885 robust_rms_before=0.904 arcsec robust_rms_before_corrected=0.337 arcsec robust_rms_after=0.357 arcsec worst_region_rms_before=0.447 worst_region_rms_after=0.436 outer_annulus_rms_before=1.191 outer_annulus_rms_after=0.436
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.447 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits worst_region_rms_kept=0.447 arcsec robust_rms_kept=0.337 arcsec matched=4885
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits N_match=4885 sigma_overall_arcsec=0.356 sigma_q1_arcsec=0.338 sigma_q2_arcsec=0.360 sigma_q3_arcsec=0.373 sigma_q4_arcsec=0.348 n_q1=1523 n_q2=1020 n_q3=1496 n_q4=846 worst_quadrant_to_overall_ratio=1.047
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits -region wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.G3KMJRJiiM (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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=418, bad_region=2109, passed=8246
Got 8246 stars (including 5806 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat
util/solve_plate_with_UCAC5 got 8246 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 6567 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 6567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 6567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4886 stars left (next iteration limit 5374)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4886 robust_rms=7.607 arcsec worst_region_rms=14.025 arcsec outer_annulus_rms=14.025 arcsec
SIP_REFIT: SIP order 3 trial: matched=4886 robust_rms=0.492 arcsec worst_region_rms=1.044 arcsec outer_annulus_rms=1.044 arcsec
SIP_REFIT: SIP order 5 trial: matched=4886 robust_rms=0.356 arcsec worst_region_rms=0.436 arcsec outer_annulus_rms=0.436 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4886 robust_rms_before=0.880 arcsec robust_rms_before_corrected=0.340 arcsec robust_rms_after=0.356 arcsec worst_region_rms_before=0.442 worst_region_rms_after=0.436 outer_annulus_rms_before=1.206 outer_annulus_rms_after=0.436
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.442 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits worst_region_rms_kept=0.442 arcsec robust_rms_kept=0.340 arcsec matched=4886
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits N_match=4886 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.377 sigma_q4_arcsec=0.369 n_q1=1533 n_q2=1010 n_q3=1485 n_q4=858 worst_quadrant_to_overall_ratio=1.048
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits -region wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits to local_wcs_cache/
'wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits' -> 'local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits'
Saving the final (post-refit) wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits to local_wcs_cache/
'wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits' -> 'local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits'
Saving the final (post-refit) wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits'
Saving the final (post-refit) wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits sigma_overall=0.355 worst_q_ratio=1.140
ref2=Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits sigma_overall=0.358 worst_q_ratio=1.106
new1=fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits sigma_overall=0.356 worst_q_ratio=1.047
new2=fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits sigma_overall=0.359 worst_q_ratio=1.048
reference average sigma_overall=0.3565 worst_q_ratio=1.123
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963_astrometric_residuals.png (4852 matched stars from wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432_astrometric_residuals.png (4854 matched stars from wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386_astrometric_residuals.png (4885 matched stars from wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387_astrometric_residuals.png (4886 matched stars from wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits'
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits'
Preparing the HTML report for the field Peg-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:59:51.03 +15:00:26.4: 12.41 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:58:54.48 +14:51:45.5: 12.66 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:59:56.26 +14:18:11.5: 12.85 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:59:51.03 +15:00:26.4: 12.40 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:59:56.26 +14:18:11.5: 12.35 +/- 0.01 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:58:54.48 +14:51:45.5: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter REJECTED candidate at 22:59:51.03 +15:00:26.4: ref_mag=12.40 +/- 0.01 new_mean_mag=12.3639 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:59:56.26 +14:18:11.5: ref_mag=12.51 +/- 0.01 new_mean_mag=12.3114 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 22:58:54.48 +14:51:45.5: ref_mag=12.44 +/- 0.01 new_mean_mag=12.2255 delta=0.21 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21504_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 21504_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21568_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 21568_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21632_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 21632_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Peg-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.cat to cache
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Creating symlink local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits exists and is non-empty
wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits exists and is non-empty
wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits exists and is non-empty
wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (1st reference image)
verification OK: wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:39.243 +14:00:09.40 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:39.416 +14:00:08.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:39.243 +14:00:09.40
Second-epoch image center 23:06:39.416 +14:00:08.23
Angular distance between the image centers 0.0008 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:36.885 +13:59:33.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:39.243 +14:00:09.40
Second-epoch image center 23:06:36.885 +13:59:33.28
Angular distance between the image centers 0.0138 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:06:39.416 +14:00:08.23
Second-epoch second image center 23:06:36.885 +13:59:33.28
Angular distance between the image centers 0.01410 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits &> /tmp/tmp.jBbBOa7bkA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits &> /tmp/tmp.icK2SPY8MI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits &> /tmp/tmp.nIEK3KUpgz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits &> /tmp/tmp.wuCOD8WGmN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
Found non-empty wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
The reference image (wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits) and catalog (wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat) found
'wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat' -> 'wcsmag.cat'
Read 52987 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3668 to 354.8803 deg, Dec +8.6362 to +19.2696 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 338.3668 to 354.8803 deg, Dec 8.6362 to 19.2696 deg
Loaded 5972 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): 4571 out of 5107 total matches.
Matched with Tycho-2 5107 out of 52987 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.563000
a=0.000000 b=1.000000 c=22.563000
From vast_summary.log: estimated ref. image limiting mag.: -6.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.67
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.67
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 52987 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3668 to 354.8803 deg, Dec +8.6362 to +19.2696 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 338.3668 to 354.8803 deg, Dec 8.6362 to 19.2696 deg
Loaded 5972 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): 4571 out of 5107 total matches.
Matched with Tycho-2 5107 out of 52987 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (aperture=4.8)
Read 51434 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3689 to 354.8805 deg, Dec +8.6361 to +19.2674 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 338.3689 to 354.8805 deg, Dec 8.6361 to 19.2674 deg
Loaded 5969 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): 4607 out of 5108 total matches.
Matched with Tycho-2 5108 out of 51434 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 31 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
2.1 pix Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
2.2 pix fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
2.2 pix fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Limiting magnitude estimates:
15.7 mag. Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
15.6 mag. Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
15.5 mag. fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
15.5 mag. fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jBbBOa7bkA (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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits' -> 'wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=2646, bad_region=8866, passed=52964
Got 52964 stars (including 41820 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
util/solve_plate_with_UCAC5 got 52964 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 4853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 46371 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 46371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 46371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4852 stars left (next iteration limit 5338)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits N_match=4852 sigma_overall_arcsec=0.348 sigma_q1_arcsec=0.308 sigma_q2_arcsec=0.335 sigma_q3_arcsec=0.390 sigma_q4_arcsec=0.332 n_q1=1534 n_q2=856 n_q3=1639 n_q4=823 worst_quadrant_to_overall_ratio=1.122
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits -region wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.icK2SPY8MI (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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits' -> 'wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2452, bad_region=8445, passed=51421
Got 51421 stars (including 40876 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat
util/solve_plate_with_UCAC5 got 51421 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 45129 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 45129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 45129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4850 stars left (next iteration limit 5335)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits N_match=4850 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.316 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.343 n_q1=1529 n_q2=849 n_q3=1654 n_q4=818 worst_quadrant_to_overall_ratio=1.088
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits -region wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.nIEK3KUpgz (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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2430, bad_region=8490, passed=46291
Got 46291 stars (including 36125 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat
util/solve_plate_with_UCAC5 got 46291 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 4879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 39940 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 39940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 39940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4879 stars left (next iteration limit 5366)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4879 robust_rms=7.523 arcsec worst_region_rms=14.163 arcsec outer_annulus_rms=14.163 arcsec
SIP_REFIT: SIP order 3 trial: matched=4879 robust_rms=0.476 arcsec worst_region_rms=1.161 arcsec outer_annulus_rms=1.161 arcsec
SIP_REFIT: SIP order 5 trial: matched=4879 robust_rms=0.353 arcsec worst_region_rms=0.435 arcsec outer_annulus_rms=0.435 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4879 robust_rms_before=0.900 arcsec robust_rms_before_corrected=0.334 arcsec robust_rms_after=0.353 arcsec worst_region_rms_before=0.434 worst_region_rms_after=0.435 outer_annulus_rms_before=1.182 outer_annulus_rms_after=0.435
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.434 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits worst_region_rms_kept=0.434 arcsec robust_rms_kept=0.334 arcsec matched=4879
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits N_match=4879 sigma_overall_arcsec=0.347 sigma_q1_arcsec=0.334 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.363 sigma_q4_arcsec=0.336 n_q1=1516 n_q2=1021 n_q3=1490 n_q4=852 worst_quadrant_to_overall_ratio=1.048
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits -region wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.wuCOD8WGmN (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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2398, bad_region=8468, passed=46287
Got 46287 stars (including 36155 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat
util/solve_plate_with_UCAC5 got 46287 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 39974 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 39974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 39974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4878 stars left (next iteration limit 5365)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4878 robust_rms=7.504 arcsec worst_region_rms=14.466 arcsec outer_annulus_rms=14.466 arcsec
SIP_REFIT: SIP order 3 trial: matched=4878 robust_rms=0.480 arcsec worst_region_rms=1.155 arcsec outer_annulus_rms=1.155 arcsec
SIP_REFIT: SIP order 5 trial: matched=4878 robust_rms=0.352 arcsec worst_region_rms=0.431 arcsec outer_annulus_rms=0.431 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4878 robust_rms_before=0.876 arcsec robust_rms_before_corrected=0.332 arcsec robust_rms_after=0.352 arcsec worst_region_rms_before=0.434 worst_region_rms_after=0.431 outer_annulus_rms_before=1.197 outer_annulus_rms_after=0.431
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.434 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits worst_region_rms_kept=0.434 arcsec robust_rms_kept=0.332 arcsec matched=4878
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits N_match=4878 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.335 sigma_q2_arcsec=0.346 sigma_q3_arcsec=0.367 sigma_q4_arcsec=0.356 n_q1=1531 n_q2=1011 n_q3=1486 n_q4=850 worst_quadrant_to_overall_ratio=1.049
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits -region wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-50-25_20.00sec_0.00C_LIGHT_0386.fits
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.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_2026-10-07_CI_Peg-10-Q2b1x1_093608_TTUQ2b1x1_3226350_JSfoQdFT/wcs_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387.fits
Preparing the HTML report for the field Peg-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:24:04.45 +16:58:21.1: 14.77 +/- 0.12 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:54:43.01 +16:58:18.1: 12.08 +/- 0.01 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:09:04.75 +10:56:07.4: 14.37 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:50:58.55 +16:18:08.1: 14.76 +/- 0.12 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:12:07.39 +14:25:39.0: 14.13 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:17:07.98 +14:12:17.5: 14.77 +/- 0.11 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:59:17.01 +18:06:44.0: 14.94 +/- 0.13 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:19:51.75 +10:57:28.0: 13.88 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:48:10.95 +17:11:57.6: 13.91 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:13:04.92 +11:31:43.6: 14.83 +/- 0.12 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:19:51.75 +10:57:28.0: 13.89 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:24:04.45 +16:58:21.1: 14.66 +/- 0.11 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:54:43.01 +16:58:18.1: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Forced photometry reference-image weighted average: 14.71 +/- 0.08
Forced photometry filter REJECTED candidate at 23:19:51.75 +10:57:28.0: ref_mag=13.88 +/- 0.04 new_mean_mag=14.1274 delta=-0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:24:04.45 +16:58:21.1: ref_mag=14.71 +/- 0.08 new_mean_mag=14.7320 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:17:07.98 +14:12:17.5: 14.76 +/- 0.11 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:09:04.75 +10:56:07.4: 14.41 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:50:58.55 +16:18:08.1: 14.68 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter REJECTED candidate at 22:54:43.01 +16:58:18.1: ref_mag=12.07 +/- 0.01 new_mean_mag=12.0362 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.39 +/- 0.06
Forced photometry filter REJECTED candidate at 23:09:04.75 +10:56:07.4: ref_mag=14.39 +/- 0.06 new_mean_mag=14.3927 delta=-0.00 (need > 0.90)
Forced photometry reference-image weighted average: 14.72 +/- 0.09
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:13:04.92 +11:31:43.6: 14.76 +/- 0.12 detection
Forced photometry filter REJECTED candidate at 22:50:58.55 +16:18:08.1: ref_mag=14.72 +/- 0.09 new_mean_mag=14.8829 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 14.77 +/- 0.08
Forced photometry filter REJECTED candidate at 23:17:07.98 +14:12:17.5: ref_mag=14.77 +/- 0.08 new_mean_mag=14.8702 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:12:07.39 +14:25:39.0: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.08
Forced photometry filter REJECTED candidate at 23:13:04.92 +11:31:43.6: ref_mag=14.79 +/- 0.08 new_mean_mag=14.6780 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:48:10.95 +17:11:57.6: 13.79 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:59:17.01 +18:06:44.0: 14.98 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 23:12:07.39 +14:25:39.0: ref_mag=14.12 +/- 0.04 new_mean_mag=14.3399 delta=-0.22 (need > 0.90)
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Forced photometry filter REJECTED candidate at 22:48:10.95 +17:11:57.6: ref_mag=13.85 +/- 0.04 new_mean_mag=14.1744 delta=-0.33 (need > 0.90)
Forced photometry reference-image weighted average: 14.96 +/- 0.10
Forced photometry filter REJECTED candidate at 22:59:17.01 +18:06:44.0: ref_mag=14.96 +/- 0.10 new_mean_mag=14.7782 delta=0.18 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:10:54.39 +16:47:17.6: 14.04 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:52:34.54 +13:40:58.4: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:05:07.19 +16:28:14.8: 14.01 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:23:07.07 +10:47:44.3: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:13:38.05 +14:11:10.3: 14.65 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:07:19.70 +16:34:46.2: 14.66 +/- 0.12 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:01:41.04 +14:44:30.9: 14.89 +/- 0.14 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:50:57.88 +17:38:34.8: 14.01 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:55:53.31 +14:21:49.6: 13.85 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:05:07.19 +16:28:14.8: 14.07 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:52:34.54 +13:40:58.4: 15.95 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Forced photometry filter REJECTED candidate at 23:05:07.19 +16:28:14.8: ref_mag=14.04 +/- 0.05 new_mean_mag=14.3787 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:10:54.39 +16:47:17.6: 14.12 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:13:38.05 +14:11:10.3: 14.55 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.04
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:23:07.07 +10:47:44.3: 15.97 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:10:54.39 +16:47:17.6: ref_mag=14.07 +/- 0.04 new_mean_mag=14.0075 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 14.59 +/- 0.07
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:07:19.70 +16:34:46.2: 14.99 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 23:13:38.05 +14:11:10.3: ref_mag=14.59 +/- 0.07 new_mean_mag=14.5518 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.77 +/- 0.09
Forced photometry filter REJECTED candidate at 23:07:19.70 +16:34:46.2: ref_mag=14.77 +/- 0.09 new_mean_mag=14.5531 delta=0.21 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:01:41.04 +14:44:30.9: 14.97 +/- 0.16 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:50:57.88 +17:38:34.8: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.10
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Forced photometry filter REJECTED candidate at 23:01:41.04 +14:44:30.9: ref_mag=14.93 +/- 0.10 new_mean_mag=14.6762 delta=0.25 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:55:53.31 +14:21:49.6: 13.94 +/- 0.06 detection
Forced photometry filter REJECTED candidate at 22:50:57.88 +17:38:34.8: ref_mag=14.05 +/- 0.05 new_mean_mag=14.2384 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Forced photometry filter REJECTED candidate at 22:55:53.31 +14:21:49.6: ref_mag=13.89 +/- 0.04 new_mean_mag=14.1824 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:23:50.28 +09:48:24.9: 15.05 +/- 0.15 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:23:50.28 +09:48:24.9: 15.53 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.13
Forced photometry filter REJECTED candidate at 23:23:50.28 +09:48:24.9: ref_mag=15.19 +/- 0.13 new_mean_mag=14.8870 delta=0.30 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:25:11.62 +17:45:14.7: 14.96 +/- 0.14 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:12:58.08 +17:07:36.4: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:22:32.31 +11:37:02.0: 15.24 +/- 0.17 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:11:43.18 +10:29:37.4: 15.55 +/- 0.22 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:48:39.27 +16:15:55.3: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:22:54.00 +10:17:41.2: 15.24 +/- 0.17 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:08:46.36 +15:32:15.0: 14.84 +/- 0.13 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:25:11.62 +17:45:14.7: 14.85 +/- 0.13 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:12:58.08 +17:07:36.4: 16.02 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.90 +/- 0.10
Forced photometry filter REJECTED candidate at 23:25:11.62 +17:45:14.7: ref_mag=14.90 +/- 0.10 new_mean_mag=14.9450 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:22:32.31 +11:37:02.0: 15.48 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.13
Forced photometry filter REJECTED candidate at 23:22:32.31 +11:37:02.0: ref_mag=15.33 +/- 0.13 new_mean_mag=14.9534 delta=0.37 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:48:39.27 +16:15:55.3: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:22:54.00 +10:17:41.2: 15.10 +/- 0.16 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:11:43.18 +10:29:37.4: 15.29 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.17 +/- 0.11
Forced photometry reference-image weighted average: 15.40 +/- 0.14
Forced photometry filter REJECTED candidate at 23:22:54.00 +10:17:41.2: ref_mag=15.17 +/- 0.11 new_mean_mag=14.9077 delta=0.26 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:08:46.36 +15:32:15.0: 14.93 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 23:11:43.18 +10:29:37.4: ref_mag=15.40 +/- 0.14 new_mean_mag=14.9917 delta=0.41 (need > 0.90)
Forced photometry reference-image weighted average: 14.88 +/- 0.10
Forced photometry filter REJECTED candidate at 23:08:46.36 +15:32:15.0: ref_mag=14.88 +/- 0.10 new_mean_mag=14.9650 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:49:46.97 +14:20:56.8: 15.45 +/- 0.21 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:49:46.97 +14:20:56.8: 15.31 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.38 +/- 0.15
Forced photometry filter REJECTED candidate at 22:49:46.97 +14:20:56.8: ref_mag=15.38 +/- 0.15 new_mean_mag=15.0182 delta=0.36 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:12:22.62 +10:06:04.5: 15.32 +/- 0.18 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:02:16.71 +10:26:28.6: 15.18 +/- 0.17 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:12:22.62 +10:06:04.5: 16.02 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.32 +/- 0.18
Forced photometry filter REJECTED candidate at 23:12:22.62 +10:06:04.5: ref_mag=15.32 +/- 0.18 new_mean_mag=15.0528 delta=0.27 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:02:16.71 +10:26:28.6: 15.43 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.27 +/- 0.14
Forced photometry filter REJECTED candidate at 23:02:16.71 +10:26:28.6: ref_mag=15.27 +/- 0.14 new_mean_mag=14.9427 delta=0.32 (need > 0.90)
Adding exclusion_list_local.txt__out68903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74162.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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: 4s
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Considering the candidate 65767_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 65767_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 65768_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 65768_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 65770_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 65770_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 65774_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 65774_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 65776_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 65776_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 65788_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 65788_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 65790_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 65790_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 65792_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 65792_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 65793_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 65793_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 66833_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 66833_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 68903_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
Preparing report for the candidate 68903_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
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Considering the candidate 70300_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 70300_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 70548_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
Preparing report for the candidate 70548_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
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Considering the candidate 70572_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 70572_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
**** FOUND 22:52:33.13 +10:20:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71170_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 71170_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 71755_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 71755_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 71818_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 71818_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 72111_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 72111_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 72286_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 72286_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 72893_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 72893_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 73707_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 73707_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 73730_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 73730_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 73796_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 73796_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 73820_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 73820_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 73871_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
Preparing report for the candidate 73871_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
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Considering the candidate 73908_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 73908_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 73975_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 73975_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 74162_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
Preparing report for the candidate 74162_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
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Considering the candidate 74169_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 74169_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 74258_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 74258_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks
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Considering the candidate 74345_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387
The candidate 74345_fd_Peg-10-Q2b1x1_2026-10-07_03-51-36_20.00sec_-0.00C_LIGHT_0387 did not pass the final checks