This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J
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 06 18.3537 2461209.8537 12.71 00:00:32.37 +13:06:42.4
104.26766 -47.90691 galactic Peg Second-epoch detections are separated by 0.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.71 Niobe -1 -0 1 12.9 0 0
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 00:00:32.37 +13:06:42.4: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 00:00:32.37 +13:06:42.4: 16.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.8537,12.71,0.05,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 20260618.3537 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3537 2461209.8537 13.42 00:12:15.02 +09:58:14.5
107.24286 -51.70334 galactic Psc Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.165 Loreley -0 0 1 13.5 0 0
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 00:12:15.02 +09:58:14.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 00:12:15.02 +09:58:14.5: 15.93 +/- 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,2461209.8537,13.42,0.05,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 20260618.3537 13.42CV 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 06 18.3537 2461209.8537 13.97 00:05:13.17 +18:16:03.2
107.79627 -43.24173 galactic Peg Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.726 Joella -1 0 1 14.6 0 0
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 00:05:13.17 +18:16:03.2: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 00:05:13.17 +18:16:03.2: 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,2461209.8537,13.97,0.05,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 20260618.3537 13.97CV 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 06 18.3537 2461209.8537 14.45 23:57:29.68 +11:36:23.3
102.50610 -49.11406 galactic Peg Second-epoch detections are separated by 2.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.665 Sabine -1 -1 1 14.4 -0 -0
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 23:57:29.68 +11:36:23.3: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 23:57:29.68 +11:36:23.3: 16.07 +/- 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,2461209.8537,14.45,0.05,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 20260618.3537 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.61599738 09.01.2026 02:46:52.174 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
First image: 2461049.61599738 09.01.2026 02:46:52.174 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
Last image: 2461209.85399355 18.06.2026 08:29:35.043 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6324
Objects passed selection criteria: 6298
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 4803.75
Average stars matched: 4437 (92.3653 %)
Memory usage VmPeak: 111820 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 18 07:46:02 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.61599738 09.01.2026 02:46:52.174 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
First image: 2461049.61599738 09.01.2026 02:46:52.174 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
Last image: 2461209.85399355 18.06.2026 08:29:35.043 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 21 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 37904
Objects passed selection criteria: 37782
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: 29377
Average stars matched: 26824.2 (91.3104 %)
Memory usage VmPeak: 136740 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 18 07:48:29 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 --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
SExtractor catalog cache: saved Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.cat to cache
SExtractor catalog cache: saved Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.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-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461209.85348903
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-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits exists and is non-empty
Saving wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits to local_wcs_cache/
'wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits' -> 'local_wcs_cache/wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits'
wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits exists and is non-empty
Saving wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits to local_wcs_cache/
'wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits' -> 'local_wcs_cache/wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits'
wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits exists and is non-empty
Saving wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits to local_wcs_cache/
'wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits' -> 'local_wcs_cache/wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits'
wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits exists and is non-empty
Saving wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits to local_wcs_cache/
'wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits' -> 'local_wcs_cache/wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits (1st reference image)
verification OK: wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
Image size: 934.5'x631.1' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.93"/pix along the Y axis
Image center: 00:00:03.825 +14:00:14.73 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/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-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits (1st new image)
verification OK: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
Image size: 938.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:52.360 +14:00:28.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:03.825 +14:00:14.73
Second-epoch image center 23:59:52.360 +14:00:28.48
Angular distance between the image centers 0.0465 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits (2nd new image)
verification OK: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
Image size: 938.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:50.066 +14:00:16.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:03.825 +14:00:14.73
Second-epoch image center 23:59:50.066 +14:00:16.23
Angular distance between the image centers 0.0556 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:52.360 +14:00:28.48
Second-epoch second image center 23:59:50.066 +14:00:16.23
Angular distance between the image centers 0.00988 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits &> /tmp/tmp.UAcIiG27r8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits &> /tmp/tmp.XhPMoHoWm7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits &> /tmp/tmp.EImshDs3K7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits &> /tmp/tmp.IWoqZrJznD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.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-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits and wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.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-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits and wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat
Found non-empty wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits and wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat
The reference image (wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits) and catalog (wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat) found
'wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat' -> 'wcsmag.cat'
Read 7349 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 360.0000 deg, Dec +8.6199 to +19.2511 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 0.0003 to 360.0000 deg, Dec 8.6199 to 19.2511 deg
Loaded 178448 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): 67 out of 71 total matches.
Matched with Tycho-2 71 out of 7349 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.901700
a=0.000000 b=1.000000 c=22.901700
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7349 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 360.0000 deg, Dec +8.6199 to +19.2511 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 0.0003 to 360.0000 deg, Dec 8.6199 to 19.2511 deg
Loaded 178448 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): 67 out of 71 total matches.
Matched with Tycho-2 71 out of 7349 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits:
Forced-photometry filter: calibrated wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits -> calib.txt_param_ref_wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits (aperture=5.9)
Read 7196 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0042 to 359.9992 deg, Dec +8.6536 to +19.2851 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 0.0042 to 359.9992 deg, Dec 8.6536 to 19.2851 deg
Loaded 178360 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): 4263 out of 4456 total matches.
Matched with Tycho-2 4456 out of 7196 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits:
Forced-photometry filter: calibrated wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits -> calib.txt_param_ref_wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
2.0 pix Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
2.3 pix fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
2.3 pix fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
2.1 pix wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
2.0 pix wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
Limiting magnitude estimates:
15.3 mag. Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
15.3 mag. Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
14.7 mag. fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
14.7 mag. fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.UAcIiG27r8 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.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-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits' -> 'wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
WCS-calibrated image found: wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
Checking if the catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat corresponding to the image wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat corresponding to the image wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
WCS catalog name: wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=467, passed=7349
Got 7349 stars (including 6878 good ones) from the SExtractor catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat
util/solve_plate_with_UCAC5 got 7349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 934.5'
Seting catalog search parameters based on the expected field of view 934.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012979 (46.7 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010383 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9607 through 0 to 8.3771, gap 8.3771 to 351.9607
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 253 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 235 matched stars entering correct_measured_positions(), 210 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.14"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 231 matched stars entering correct_measured_positions(), 1751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.16"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9631 through 0 to 8.3674, gap 8.3674 to 351.9631
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 318 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 300 matched stars entering correct_measured_positions(), 1792 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.01"
Accuracy estimation diagnostic: 300 matched stars entering correct_measured_positions(), 2272 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.50"
Excluding outliers - 300 stars left (next iteration limit 254)
WCS_QUALITY_DIAG: file=Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits N_match=300 sigma_overall_arcsec=5.543 sigma_q1_arcsec=5.012 sigma_q2_arcsec=23.740 sigma_q3_arcsec=4.999 sigma_q4_arcsec=28.028 n_q1=153 n_q2=6 n_q3=134 n_q4=7 worst_quadrant_to_overall_ratio=5.056
The image catalog is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits -region wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.XhPMoHoWm7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.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-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits' -> 'wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
WCS_IMAGE_NAME=wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
WCS-calibrated image found: wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
Checking if the catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat corresponding to the image wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits alredy exist and is non-empty...
Catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat corresponding to the image wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
WCS catalog name: wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=462, passed=7196
Got 7196 stars (including 6728 good ones) from the SExtractor catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat
util/solve_plate_with_UCAC5 got 7196 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7849 through 0 to 8.3280, gap 8.3280 to 351.7849
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 7119 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
RA wraps around 0/360 boundary: field RA 351.7845 through 0 to 8.3285, gap 8.3285 to 351.7845
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 7116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 7116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits N_match=980 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.439 sigma_q2_arcsec=0.277 sigma_q3_arcsec=0.312 sigma_q4_arcsec=0.276 n_q1=233 n_q2=286 n_q3=200 n_q4=261 worst_quadrant_to_overall_ratio=1.397
The image catalog is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits -region wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EImshDs3K7 (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_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.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_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
WCS_IMAGE_NAME=wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
WCS-calibrated image found: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
Checking if the catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat corresponding to the image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat corresponding to the image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
WCS catalog name: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=255, passed=5266
Got 5266 stars (including 5003 good ones) from the SExtractor catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat
util/solve_plate_with_UCAC5 got 5266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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
RA wraps around 0/360 boundary: field RA 351.6811 through 0 to 8.1314, gap 8.1314 to 351.6811
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.6807 through 0 to 8.1316, gap 8.1316 to 351.6807
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits N_match=979 sigma_overall_arcsec=0.416 sigma_q1_arcsec=0.401 sigma_q2_arcsec=0.454 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.496 n_q1=269 n_q2=203 n_q3=239 n_q4=268 worst_quadrant_to_overall_ratio=1.192
The image catalog is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits -region wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IWoqZrJznD (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_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.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_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
WCS_IMAGE_NAME=wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
WCS-calibrated image found: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
Checking if the catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat corresponding to the image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat corresponding to the image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
WCS catalog name: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=285, passed=5329
Got 5329 stars (including 5040 good ones) from the SExtractor catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat
util/solve_plate_with_UCAC5 got 5329 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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
RA wraps around 0/360 boundary: field RA 351.6811 through 0 to 8.1315, gap 8.1315 to 351.6811
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 5270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.6807 through 0 to 8.1317, gap 8.1317 to 351.6807
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 5268 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 5268 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits N_match=982 sigma_overall_arcsec=0.414 sigma_q1_arcsec=0.383 sigma_q2_arcsec=0.471 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.508 n_q1=264 n_q2=206 n_q3=247 n_q4=265 worst_quadrant_to_overall_ratio=1.225
The image catalog is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits -region wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits sigma_overall=5.543 worst_q_ratio=5.056
ref2=Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits sigma_overall=0.314 worst_q_ratio=1.397
new1=fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits sigma_overall=0.416 worst_q_ratio=1.192
new2=fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits sigma_overall=0.414 worst_q_ratio=1.225
reference average sigma_overall=2.9285 worst_q_ratio=3.2265
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059_astrometric_residuals.png (300 matched stars from wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.06 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060_astrometric_residuals.png (980 matched stars from wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328_astrometric_residuals.png (979 matched stars from wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329_astrometric_residuals.png (982 matched stars from wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits'
Saving fully-calibrated image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits'
Preparing the HTML report for the field Peg-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 00:02:30.73 +14:02:50.3: 14.84 +/- 0.13 detection
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 00:02:30.73 +14:02:50.3: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry filter REJECTED candidate at 00:02:30.73 +14:02:50.3: ref_mag=12.10 +/- 0.01 new_mean_mag=12.0627 delta=0.04 (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 21245_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
The candidate 21245_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329 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-07-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 --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
SExtractor catalog cache: saved Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.cat to cache
SExtractor catalog cache: saved Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.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-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
Creating symlink local_wcs_cache/wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits exists and is non-empty
wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits exists and is non-empty
wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits exists and is non-empty
wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits (1st reference image)
verification OK: wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
Image size: 934.5'x631.1' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.93"/pix along the Y axis
Image center: 00:00:03.825 +14:00:14.73 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/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-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits (1st new image)
verification OK: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
Image size: 938.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:52.360 +14:00:28.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:03.825 +14:00:14.73
Second-epoch image center 23:59:52.360 +14:00:28.48
Angular distance between the image centers 0.0465 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits (2nd new image)
verification OK: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
Image size: 938.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:50.066 +14:00:16.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:03.825 +14:00:14.73
Second-epoch image center 23:59:50.066 +14:00:16.23
Angular distance between the image centers 0.0556 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:59:52.360 +14:00:28.48
Second-epoch second image center 23:59:50.066 +14:00:16.23
Angular distance between the image centers 0.00988 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits &> /tmp/tmp.eaUD7sPONW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits &> /tmp/tmp.zplBoTbvSl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits &> /tmp/tmp.rhNZJtEeKh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits &> /tmp/tmp.BTPIPYIj6q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.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-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits and wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.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-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits and wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat
Found non-empty wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits and wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat
The reference image (wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits) and catalog (wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat) found
'wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat' -> 'wcsmag.cat'
Read 41576 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 360.0000 deg, Dec +8.5542 to +19.2522 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 0.0003 to 360.0000 deg, Dec 8.5542 to 19.2522 deg
Loaded 179601 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): 74 out of 81 total matches.
Matched with Tycho-2 81 out of 41576 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.765750
a=0.000000 b=1.000000 c=22.765750
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 41576 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 360.0000 deg, Dec +8.5542 to +19.2522 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 0.0003 to 360.0000 deg, Dec 8.5542 to 19.2522 deg
Loaded 179601 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): 74 out of 81 total matches.
Matched with Tycho-2 81 out of 41576 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits:
Forced-photometry filter: calibrated wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits -> calib.txt_param_ref_wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits (aperture=4.7)
Read 42454 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0010 to 359.9992 deg, Dec +8.5963 to +19.2873 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 0.0010 to 359.9992 deg, Dec 8.5963 to 19.2873 deg
Loaded 179419 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): 4197 out of 4609 total matches.
Matched with Tycho-2 4609 out of 42454 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits:
Forced-photometry filter: calibrated wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits -> calib.txt_param_ref_wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
1.9 pix Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
2.3 pix fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
2.2 pix fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
2.0 pix wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
1.9 pix wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
Limiting magnitude estimates:
15.4 mag. Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
15.4 mag. Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
14.8 mag. fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
14.8 mag. fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.eaUD7sPONW (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.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-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits' -> 'wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
WCS-calibrated image found: wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
Checking if the catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat corresponding to the image wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat corresponding to the image wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits
WCS catalog name: wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1729, passed=41560
Got 41560 stars (including 39753 good ones) from the SExtractor catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat
util/solve_plate_with_UCAC5 got 41560 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 934.5'
Seting catalog search parameters based on the expected field of view 934.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012979 (46.7 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010383 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9419 through 0 to 8.3870, gap 8.3870 to 351.9419
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 254 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 238 matched stars entering correct_measured_positions(), 215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 11069 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9422 through 0 to 8.3757, gap 8.3757 to 351.9422
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 316 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 298 matched stars entering correct_measured_positions(), 11102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.21"
Accuracy estimation diagnostic: 298 matched stars entering correct_measured_positions(), 13875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.12"
Excluding outliers - 298 stars left (next iteration limit 256)
WCS_QUALITY_DIAG: file=Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits N_match=298 sigma_overall_arcsec=5.380 sigma_q1_arcsec=5.013 sigma_q2_arcsec=24.149 sigma_q3_arcsec=5.232 sigma_q4_arcsec=27.575 n_q1=152 n_q2=7 n_q3=134 n_q4=5 worst_quadrant_to_overall_ratio=5.125
The image catalog is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits -region wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zplBoTbvSl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.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-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits' -> 'wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
WCS_IMAGE_NAME=wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
WCS-calibrated image found: wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
Checking if the catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat corresponding to the image wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits alredy exist and is non-empty...
Catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat corresponding to the image wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits
WCS catalog name: wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1724, passed=42439
Got 42439 stars (including 40649 good ones) from the SExtractor catalog wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat
util/solve_plate_with_UCAC5 got 42439 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7713 through 0 to 8.3484, gap 8.3484 to 351.7713
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 42028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7711 through 0 to 8.3489, gap 8.3489 to 351.7711
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 42027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 42027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits N_match=979 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.257 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.279 n_q1=237 n_q2=277 n_q3=211 n_q4=254 worst_quadrant_to_overall_ratio=1.380
The image catalog is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits -region wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rhNZJtEeKh (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_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.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_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
WCS_IMAGE_NAME=wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
WCS-calibrated image found: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
Checking if the catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat corresponding to the image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat corresponding to the image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
WCS catalog name: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1023, passed=29380
Got 29380 stars (including 28317 good ones) from the SExtractor catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat
util/solve_plate_with_UCAC5 got 29380 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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
RA wraps around 0/360 boundary: field RA 351.6155 through 0 to 8.1314, gap 8.1314 to 351.6155
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 29127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.6149 through 0 to 8.1316, gap 8.1316 to 351.6149
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 29126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 29126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits N_match=979 sigma_overall_arcsec=0.393 sigma_q1_arcsec=0.375 sigma_q2_arcsec=0.508 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.463 n_q1=263 n_q2=201 n_q3=245 n_q4=270 worst_quadrant_to_overall_ratio=1.290
The image catalog is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits -region wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BTPIPYIj6q (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_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.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_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
WCS_IMAGE_NAME=wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
WCS-calibrated image found: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
Checking if the catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat corresponding to the image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat corresponding to the image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
WCS catalog name: wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1074, passed=29637
Got 29637 stars (including 28527 good ones) from the SExtractor catalog wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat
util/solve_plate_with_UCAC5 got 29637 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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
RA wraps around 0/360 boundary: field RA 351.6043 through 0 to 8.1315, gap 8.1315 to 351.6043
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 29350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.6037 through 0 to 8.1317, gap 8.1317 to 351.6037
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 29348 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 29348 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits N_match=980 sigma_overall_arcsec=0.401 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.461 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.483 n_q1=262 n_q2=204 n_q3=247 n_q4=267 worst_quadrant_to_overall_ratio=1.204
The image catalog is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits -region wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.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_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-28-51_20.00sec_5.00C_LIGHT_0328.fits
Saving fully-calibrated image wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.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_2026-06-18_CI_Peg-07-Q2b1x1_040604_TTUQ2b1x1_1614865_FELaWo4J/wcs_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329.fits
Preparing the HTML report for the field Peg-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 00:00:32.37 +13:06:42.4: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 23:57:29.68 +11:36:23.3: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 23:49:51.64 +11:47:34.6: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 23:53:31.25 +17:56:50.2: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 00:05:13.17 +18:16:03.2: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 00:12:15.02 +09:58:14.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-46-52_20.00sec_-14.90C_LIGHT_0059.fits at 00:02:52.53 +15:11:41.6: 16.00 +/- 0.32 detection
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 23:57:29.68 +11:36:23.3: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 00:00:32.37 +13:06:42.4: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 23:49:51.64 +11:47:34.6: 15.13 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.15
Forced photometry filter REJECTED candidate at 23:49:51.64 +11:47:34.6: ref_mag=15.13 +/- 0.15 new_mean_mag=14.8135 delta=0.32 (need > 0.90)
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 23:53:31.25 +17:56:50.2: 11.11 +/- 0.00 detection
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 00:12:15.02 +09:58:14.5: 15.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Forced photometry filter REJECTED candidate at 23:53:31.25 +17:56:50.2: ref_mag=11.11 +/- 0.00 new_mean_mag=11.3034 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 00:05:13.17 +18:16:03.2: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-07-Q2b1x1_2026-01-08_20-47-38_20.00sec_-14.90C_LIGHT_0060.fits at 00:02:52.53 +15:11:41.6: 15.36 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.51 +/- 0.16
Forced photometry filter REJECTED candidate at 00:02:52.53 +15:11:41.6: ref_mag=15.51 +/- 0.16 new_mean_mag=14.7102 delta=0.80 (need > 0.90)
Adding exclusion_list_local.txt__out54540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58860.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 52632_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
The candidate 52632_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329 did not pass the final checks
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Considering the candidate 54243_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
The candidate 54243_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329 did not pass the final checks
**** FOUND 00:13:03.21 +15:11:43.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 54540_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
Preparing report for the candidate 54540_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
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Considering the candidate 55077_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
The candidate 55077_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329 did not pass the final checks
**** FOUND 00:13:02.90 +15:11:24.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 56004_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
Preparing report for the candidate 56004_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
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Considering the candidate 57344_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
Preparing report for the candidate 57344_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
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Considering the candidate 58860_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
Preparing report for the candidate 58860_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
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Considering the candidate 59493_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
The candidate 59493_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329 did not pass the final checks
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Considering the candidate 59535_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329
The candidate 59535_fd_Peg-07-Q2b1x1_2026-06-18_03-29-35_20.00sec_5.00C_LIGHT_0329 did not pass the final checks