This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg
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 18.3641 2461209.8641 14.44 22:56:57.46 +18:14:06.9
88.29874 -36.82154 galactic Peg Second-epoch detections are separated by 1.2" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.978 Aidamina -0 -0 0 14.5 -0 0
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:56:57.46 +18:14:06.9: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:56:57.46 +18:14:06.9: 15.69 +/- 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,2461209.8641,14.44,0.05,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 20260618.3641 14.44CV 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 18.3641 2461209.8641 11.47 23:20:07.08 +16:04:05.9
93.10009 -41.45351 galactic Peg Second-epoch detections are separated by 0.3" and 8.8 pix
The object was found in VSX 1" DZ Peg
Type: RRAB
# Max. Min./Amp. JD0 Period
11.325 V 12.435 V 2433891.30800 0.607344700000 A8
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:20:07.08 +16:04:05.9: 12.40 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:20:07.08 +16:04:05.9: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
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
DZ Peg,2461209.8641,11.47,0.05,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
DZ Peg 20260618.3641 11.47CV 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: 2461061.60628759 21.01.2026 02:32:53.248 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
First image: 2461061.60628759 21.01.2026 02:32:53.248 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
Last image: 2461209.86435169 18.06.2026 08:44:29.986 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 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): 7320
Objects passed selection criteria: 7287
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: 5707.75
Average stars matched: 5002 (87.6352 %)
Memory usage VmPeak: 112560 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 07:58:23 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: 2461061.60628759 21.01.2026 02:32:53.248 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
First image: 2461061.60628759 21.01.2026 02:32:53.248 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
Last image: 2461209.86435169 18.06.2026 08:44:29.986 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 87
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 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): 44526
Objects passed selection criteria: 44407
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: 35295.2
Average stars matched: 31112.5 (88.1493 %)
Memory usage VmPeak: 141148 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 08:00:24 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-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.cat to cache
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.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: 2461209.86376611
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits exists and is non-empty
Saving wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits to local_wcs_cache/
'wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits' -> 'local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits'
wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits exists and is non-empty
Saving wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits to local_wcs_cache/
'wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits' -> 'local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits'
wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits exists and is non-empty
Saving wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits'
wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits exists and is non-empty
Saving wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits (1st reference image)
verification OK: wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
Image size: 942.1'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:06:41.061 +13:59:46.03 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:25.304 +14:00:10.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:41.061 +13:59:46.03
Second-epoch image center 23:06:25.304 +14:00:10.64
Angular distance between the image centers 0.0641 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:23.473 +14:00:56.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:41.061 +13:59:46.03
Second-epoch image center 23:06:23.473 +14:00:56.85
Angular distance between the image centers 0.0738 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:06:25.304 +14:00:10.64
Second-epoch second image center 23:06:23.473 +14:00:56.85
Angular distance between the image centers 0.01482 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-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits &> /tmp/tmp.M5PtzWMj6c
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits &> /tmp/tmp.Z3KBRrvBEc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits &> /tmp/tmp.aeEI1ozKzo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits &> /tmp/tmp.Ne70Gy1B3l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits and wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits and wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
Found non-empty wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits and wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
The reference image (wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits) and catalog (wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat) found
'wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat' -> 'wcsmag.cat'
Read 7185 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4366 to 354.9948 deg, Dec +8.6296 to +19.2852 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.4366 to 354.9948 deg, Dec 8.6296 to 19.2852 deg
Loaded 5987 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): 4722 out of 4870 total matches.
Matched with Tycho-2 4870 out of 7185 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.732900
a=0.000000 b=1.000000 c=22.732900
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.98
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.98
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7185 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4366 to 354.9948 deg, Dec +8.6296 to +19.2852 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.4366 to 354.9948 deg, Dec 8.6296 to 19.2852 deg
Loaded 5987 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): 4722 out of 4870 total matches.
Matched with Tycho-2 4870 out of 7185 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits (aperture=5.8)
Read 7167 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4287 to 354.9789 deg, Dec +8.5799 to +19.2802 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.4287 to 354.9789 deg, Dec 8.5799 to 19.2802 deg
Loaded 6006 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): 4732 out of 4874 total matches.
Matched with Tycho-2 4874 out of 7167 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
2.2 pix Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
2.3 pix fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
2.4 pix fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
2.2 pix wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
2.2 pix wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
Limiting magnitude estimates:
15.0 mag. Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
15.0 mag. Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
15.0 mag. fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
15.0 mag. fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.M5PtzWMj6c (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-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.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-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits' -> 'wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=450, passed=7185
Got 7185 stars (including 6728 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 7185 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 7077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 7074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 7074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits N_match=970 sigma_overall_arcsec=0.284 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.275 sigma_q4_arcsec=0.259 n_q1=196 n_q2=295 n_q3=238 n_q4=241 worst_quadrant_to_overall_ratio=1.056
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits -region wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.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.Z3KBRrvBEc (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-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.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-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits' -> 'wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=423, passed=7167
Got 7167 stars (including 6734 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat
util/solve_plate_with_UCAC5 got 7167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 7086 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 7086 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 7086 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits N_match=971 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.305 sigma_q2_arcsec=0.308 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.298 n_q1=199 n_q2=293 n_q3=242 n_q4=237 worst_quadrant_to_overall_ratio=1.020
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits -region wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.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.aeEI1ozKzo (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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=408, passed=7810
Got 7810 stars (including 7398 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat
util/solve_plate_with_UCAC5 got 7810 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 7731 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 7734 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 7734 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits N_match=970 sigma_overall_arcsec=0.441 sigma_q1_arcsec=0.383 sigma_q2_arcsec=0.510 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.528 n_q1=247 n_q2=240 n_q3=261 n_q4=222 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits -region wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.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.Ne70Gy1B3l (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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=421, passed=7783
Got 7783 stars (including 7355 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat
util/solve_plate_with_UCAC5 got 7783 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 7698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits N_match=969 sigma_overall_arcsec=0.454 sigma_q1_arcsec=0.386 sigma_q2_arcsec=0.515 sigma_q3_arcsec=0.424 sigma_q4_arcsec=0.586 n_q1=244 n_q2=240 n_q3=265 n_q4=220 worst_quadrant_to_overall_ratio=1.291
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits -region wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.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-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits sigma_overall=0.284 worst_q_ratio=1.056
ref2=Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits sigma_overall=0.302 worst_q_ratio=1.020
new1=fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits sigma_overall=0.441 worst_q_ratio=1.196
new2=fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits sigma_overall=0.454 worst_q_ratio=1.291
reference average sigma_overall=0.293 worst_q_ratio=1.038
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070_astrometric_residuals.png (970 matched stars from wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071_astrometric_residuals.png (971 matched stars from wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342_astrometric_residuals.png (970 matched stars from wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343_astrometric_residuals.png (969 matched stars from wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits'
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits'
Preparing the HTML report for the field Peg-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:20:07.08 +16:04:06.4: 12.43 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:10:52.88 +13:44:01.4: 11.97 +/- 0.01 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:20:07.08 +16:04:06.4: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter KEPT candidate at 23:20:07.08 +16:04:06.4: ref_mag=12.44 +/- 0.01 new_mean_mag=11.5092 delta=0.93 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:10:52.88 +13:44:01.4: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter REJECTED candidate at 23:10:52.88 +13:44:01.4: ref_mag=11.98 +/- 0.01 new_mean_mag=11.9445 delta=0.04 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out21265.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 20559_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 20559_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 23:04:11.49 +15:18:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21265_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 21265_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 23:20:07.08 +16:04:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.545 2817589255885467520 350.02936218177 +16.06851757899 12.0345 11.5734 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21620_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 21620_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05970_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 05970_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 23:06:39.17 +10:32:39.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Peg-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.cat to cache
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
Creating symlink local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.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-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits exists and is non-empty
wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits exists and is non-empty
wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits exists and is non-empty
wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits (1st reference image)
verification OK: wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
Image size: 942.1'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:06:41.061 +13:59:46.03 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:25.304 +14:00:10.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:41.061 +13:59:46.03
Second-epoch image center 23:06:25.304 +14:00:10.64
Angular distance between the image centers 0.0641 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:23.473 +14:00:56.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:41.061 +13:59:46.03
Second-epoch image center 23:06:23.473 +14:00:56.85
Angular distance between the image centers 0.0738 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:06:25.304 +14:00:10.64
Second-epoch second image center 23:06:23.473 +14:00:56.85
Angular distance between the image centers 0.01482 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-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits &> /tmp/tmp.jcax43yxrD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits &> /tmp/tmp.4zwpve1BBV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits &> /tmp/tmp.go5wptvJEw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits &> /tmp/tmp.64x4ixeMaG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits and wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits and wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
Found non-empty wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits and wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
The reference image (wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits) and catalog (wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat) found
'wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat' -> 'wcsmag.cat'
Read 43173 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4144 to 355.0238 deg, Dec +8.5929 to +19.2862 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.4144 to 355.0238 deg, Dec 8.5929 to 19.2862 deg
Loaded 6024 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): 4755 out of 5179 total matches.
Matched with Tycho-2 5179 out of 43173 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.608600
a=0.000000 b=1.000000 c=22.608600
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 43173 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4144 to 355.0238 deg, Dec +8.5929 to +19.2862 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.4144 to 355.0238 deg, Dec 8.5929 to 19.2862 deg
Loaded 6024 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): 4755 out of 5179 total matches.
Matched with Tycho-2 5179 out of 43173 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits (aperture=4.6)
Read 42981 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4262 to 355.0115 deg, Dec +8.5782 to +19.2802 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.4262 to 355.0115 deg, Dec 8.5782 to 19.2802 deg
Loaded 6016 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): 4742 out of 5178 total matches.
Matched with Tycho-2 5178 out of 42981 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 53 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
2.0 pix Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
2.3 pix fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
2.3 pix fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
2.0 pix wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
2.0 pix wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
Limiting magnitude estimates:
15.1 mag. Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
15.1 mag. Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
15.2 mag. fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
15.2 mag. fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jcax43yxrD (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-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.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-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits' -> 'wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1847, passed=43167
Got 43167 stars (including 41257 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 43167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 42630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 42628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 42627 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits N_match=973 sigma_overall_arcsec=0.332 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.338 sigma_q4_arcsec=0.342 n_q1=202 n_q2=293 n_q3=245 n_q4=233 worst_quadrant_to_overall_ratio=1.030
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits -region wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.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.4zwpve1BBV (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-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.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-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits' -> 'wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1762, passed=42978
Got 42978 stars (including 41149 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat
util/solve_plate_with_UCAC5 got 42978 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 42505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 42506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 42506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits N_match=973 sigma_overall_arcsec=0.330 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.358 sigma_q4_arcsec=0.299 n_q1=203 n_q2=295 n_q3=243 n_q4=232 worst_quadrant_to_overall_ratio=1.083
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits -region wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.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.go5wptvJEw (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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=2145, passed=42245
Got 42245 stars (including 40049 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat
util/solve_plate_with_UCAC5 got 42245 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 41871 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
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 41872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 41872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits N_match=970 sigma_overall_arcsec=0.477 sigma_q1_arcsec=0.432 sigma_q2_arcsec=0.533 sigma_q3_arcsec=0.414 sigma_q4_arcsec=0.535 n_q1=241 n_q2=237 n_q3=275 n_q4=217 worst_quadrant_to_overall_ratio=1.122
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits -region wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.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.64x4ixeMaG (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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2214, passed=42331
Got 42331 stars (including 40065 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat
util/solve_plate_with_UCAC5 got 42331 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 42003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 42003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 42003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits N_match=970 sigma_overall_arcsec=0.468 sigma_q1_arcsec=0.425 sigma_q2_arcsec=0.540 sigma_q3_arcsec=0.427 sigma_q4_arcsec=0.580 n_q1=240 n_q2=238 n_q3=274 n_q4=218 worst_quadrant_to_overall_ratio=1.239
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Peg-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits -region wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.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-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-43-39_20.00sec_4.90C_LIGHT_0342.fits
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.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-10-Q2b1x1_042004_TTUQ2b1x1_974997_jZ7oyVvg/wcs_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343.fits
Preparing the HTML report for the field Peg-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:04:24.74 +11:10:51.4: 13.86 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:05:52.28 +11:48:52.4: 14.43 +/- 0.11 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:54:08.06 +17:40:58.4: 14.31 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:14:52.00 +12:38:54.0: 14.15 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:48:23.26 +14:16:58.7: 13.86 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:55:44.07 +17:57:03.3: 12.96 +/- 0.03 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:48:48.04 +11:22:07.8: 14.59 +/- 0.14 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:54:37.57 +14:04:33.4: 14.42 +/- 0.11 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:49:29.06 +11:18:09.2: 14.85 +/- 0.18 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:57:43.34 +11:31:50.3: 14.28 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:05:52.28 +11:48:52.4: 14.51 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.08
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:48:48.04 +11:22:07.8: 14.64 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 23:05:52.28 +11:48:52.4: ref_mag=14.47 +/- 0.08 new_mean_mag=14.4985 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:54:37.57 +14:04:33.4: 14.32 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:14:52.00 +12:38:54.0: 13.84 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:55:44.07 +17:57:03.3: 12.91 +/- 0.03 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:54:08.06 +17:40:58.4: 14.26 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:49:29.06 +11:18:09.2: 14.65 +/- 0.15 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:57:43.34 +11:31:50.3: 14.26 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.10
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:04:24.74 +11:10:51.4: 13.85 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:48:23.26 +14:16:58.7: 14.03 +/- 0.09 detection
Forced photometry filter REJECTED candidate at 22:48:48.04 +11:22:07.8: ref_mag=14.62 +/- 0.10 new_mean_mag=14.3598 delta=0.26 (need > 0.90)
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Forced photometry reference-image weighted average: 14.37 +/- 0.07
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry reference-image weighted average: 14.28 +/- 0.07
Forced photometry reference-image weighted average: 14.27 +/- 0.07
Forced photometry reference-image weighted average: 14.73 +/- 0.12
Forced photometry filter REJECTED candidate at 23:14:52.00 +12:38:54.0: ref_mag=13.94 +/- 0.05 new_mean_mag=14.3272 delta=-0.38 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:54:37.57 +14:04:33.4: ref_mag=14.37 +/- 0.07 new_mean_mag=14.3449 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:55:44.07 +17:57:03.3: ref_mag=12.94 +/- 0.02 new_mean_mag=13.1512 delta=-0.21 (need > 0.90)
Forced photometry reference-image weighted average: 13.86 +/- 0.06
Forced photometry filter REJECTED candidate at 22:54:08.06 +17:40:58.4: ref_mag=14.28 +/- 0.07 new_mean_mag=14.6418 delta=-0.36 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:57:43.34 +11:31:50.3: ref_mag=14.27 +/- 0.07 new_mean_mag=14.5527 delta=-0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:49:29.06 +11:18:09.2: ref_mag=14.73 +/- 0.12 new_mean_mag=14.3126 delta=0.42 (need > 0.90)
Forced photometry reference-image weighted average: 13.93 +/- 0.06
Forced photometry filter REJECTED candidate at 23:04:24.74 +11:10:51.4: ref_mag=13.86 +/- 0.06 new_mean_mag=14.1072 delta=-0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:48:23.26 +14:16:58.7: ref_mag=13.93 +/- 0.06 new_mean_mag=13.9587 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:02:58.63 +13:00:53.1: 14.40 +/- 0.10 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:48:18.06 +16:33:42.7: 14.63 +/- 0.15 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:50:30.40 +17:52:05.8: 13.73 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:54:35.75 +15:21:49.4: 14.71 +/- 0.18 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:56:57.46 +18:14:06.9: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:56:31.38 +17:47:02.1: 14.50 +/- 0.12 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:49:39.13 +12:00:16.0: 14.69 +/- 0.16 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:13:11.13 +10:46:22.1: 14.79 +/- 0.15 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:49:32.65 +09:57:27.5: 14.67 +/- 0.16 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:53:15.34 +18:02:28.7: 14.72 +/- 0.15 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:02:58.63 +13:00:53.1: 14.56 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.08
Forced photometry filter REJECTED candidate at 23:02:58.63 +13:00:53.1: ref_mag=14.47 +/- 0.08 new_mean_mag=14.4621 delta=0.00 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:54:35.75 +15:21:49.4: 14.91 +/- 0.21 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:48:18.06 +16:33:42.7: 14.34 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.14
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:50:30.40 +17:52:05.8: 14.42 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 22:54:35.75 +15:21:49.4: ref_mag=14.80 +/- 0.14 new_mean_mag=14.4634 delta=0.33 (need > 0.90)
Forced photometry reference-image weighted average: 13.89 +/- 0.07
Forced photometry reference-image weighted average: 14.45 +/- 0.09
Forced photometry filter REJECTED candidate at 22:50:30.40 +17:52:05.8: ref_mag=13.89 +/- 0.07 new_mean_mag=14.4597 delta=-0.57 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:48:18.06 +16:33:42.7: ref_mag=14.45 +/- 0.09 new_mean_mag=14.3346 delta=0.12 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:56:31.38 +17:47:02.1: 14.43 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.08
Forced photometry filter REJECTED candidate at 22:56:31.38 +17:47:02.1: ref_mag=14.46 +/- 0.08 new_mean_mag=14.4088 delta=0.06 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:56:57.46 +18:14:06.9: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:49:32.65 +09:57:27.5: 14.85 +/- 0.19 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:49:39.13 +12:00:16.0: 14.55 +/- 0.14 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:13:11.13 +10:46:22.1: 14.68 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.12
Forced photometry reference-image weighted average: 14.61 +/- 0.11
Forced photometry filter REJECTED candidate at 22:49:32.65 +09:57:27.5: ref_mag=14.74 +/- 0.12 new_mean_mag=14.3049 delta=0.44 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:49:39.13 +12:00:16.0: ref_mag=14.61 +/- 0.11 new_mean_mag=14.4918 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 14.73 +/- 0.10
Forced photometry filter REJECTED candidate at 23:13:11.13 +10:46:22.1: ref_mag=14.73 +/- 0.10 new_mean_mag=14.4526 delta=0.28 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:53:15.34 +18:02:28.7: 14.51 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.10
Forced photometry filter REJECTED candidate at 22:53:15.34 +18:02:28.7: ref_mag=14.60 +/- 0.10 new_mean_mag=14.5834 delta=0.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:56:02.24 +11:58:01.1: 14.43 +/- 0.12 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:49:39.90 +09:54:42.1: 15.12 +/- 0.24 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:52:08.66 +16:19:54.0: 14.97 +/- 0.19 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:58:32.34 +13:01:51.0: 14.63 +/- 0.12 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:50:25.60 +13:09:36.9: 15.15 +/- 0.23 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:07:17.88 +10:34:35.5: 14.73 +/- 0.15 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:58:14.87 +09:58:09.1: 14.83 +/- 0.17 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:51:55.29 +11:46:52.6: 15.12 +/- 0.23 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:56:02.24 +11:58:01.1: 14.85 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.09
Forced photometry filter REJECTED candidate at 22:56:02.24 +11:58:01.1: ref_mag=14.58 +/- 0.09 new_mean_mag=14.5553 delta=0.02 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:49:23.89 +14:38:22.4: 14.67 +/- 0.14 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:52:08.66 +16:19:54.0: 14.69 +/- 0.14 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:49:39.90 +09:54:42.1: 15.23 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.11
Forced photometry filter REJECTED candidate at 22:52:08.66 +16:19:54.0: ref_mag=14.79 +/- 0.11 new_mean_mag=14.5857 delta=0.21 (need > 0.90)
Forced photometry reference-image weighted average: 15.17 +/- 0.18
Forced photometry filter REJECTED candidate at 22:49:39.90 +09:54:42.1: ref_mag=15.17 +/- 0.18 new_mean_mag=14.5935 delta=0.58 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:50:25.60 +13:09:36.9: 15.26 +/- 0.26 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:58:32.34 +13:01:51.0: 14.52 +/- 0.11 detection
Forced photometry reference-image weighted average: 15.20 +/- 0.17
Forced photometry filter REJECTED candidate at 22:50:25.60 +13:09:36.9: ref_mag=15.20 +/- 0.17 new_mean_mag=14.6164 delta=0.58 (need > 0.90)
Forced photometry reference-image weighted average: 14.57 +/- 0.08
Forced photometry filter REJECTED candidate at 22:58:32.34 +13:01:51.0: ref_mag=14.57 +/- 0.08 new_mean_mag=14.5056 delta=0.07 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:07:17.88 +10:34:35.5: 14.76 +/- 0.16 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:58:14.87 +09:58:09.1: 14.83 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.11
Forced photometry filter REJECTED candidate at 23:07:17.88 +10:34:35.5: ref_mag=14.74 +/- 0.11 new_mean_mag=14.5481 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 14.83 +/- 0.12
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:51:55.29 +11:46:52.6: 14.62 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 22:58:14.87 +09:58:09.1: ref_mag=14.83 +/- 0.12 new_mean_mag=14.6018 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 14.76 +/- 0.12
Forced photometry filter REJECTED candidate at 22:51:55.29 +11:46:52.6: ref_mag=14.76 +/- 0.12 new_mean_mag=14.5975 delta=0.16 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:49:23.89 +14:38:22.4: 14.80 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.73 +/- 0.11
Forced photometry filter REJECTED candidate at 22:49:23.89 +14:38:22.4: ref_mag=14.73 +/- 0.11 new_mean_mag=14.6438 delta=0.09 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:52:15.34 +11:37:49.9: 14.84 +/- 0.18 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:52:08.50 +11:14:49.3: 14.60 +/- 0.14 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:49:34.44 +09:42:18.8: 14.77 +/- 0.18 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:51:26.79 +10:02:39.3: 14.63 +/- 0.15 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:52:06.25 +15:30:52.4: 14.75 +/- 0.16 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:52:21.87 +09:56:22.4: 14.89 +/- 0.19 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:51:15.96 +15:23:31.1: 14.60 +/- 0.13 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:48:38.53 +14:13:10.2: 14.94 +/- 0.19 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:52:15.34 +11:37:49.9: 15.09 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.14
Forced photometry filter REJECTED candidate at 22:52:15.34 +11:37:49.9: ref_mag=14.93 +/- 0.14 new_mean_mag=14.5954 delta=0.34 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:49:34.44 +09:42:18.8: 14.80 +/- 0.19 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:52:08.50 +11:14:49.3: 14.50 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.13
Forced photometry reference-image weighted average: 14.54 +/- 0.10
Forced photometry filter REJECTED candidate at 22:49:34.44 +09:42:18.8: ref_mag=14.79 +/- 0.13 new_mean_mag=14.5305 delta=0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:52:08.50 +11:14:49.3: ref_mag=14.54 +/- 0.10 new_mean_mag=14.6184 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:51:26.79 +10:02:39.3: 14.63 +/- 0.15 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:49:01.04 +14:10:30.9: 14.95 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.11
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:52:06.25 +15:30:52.4: 14.71 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 22:51:26.79 +10:02:39.3: ref_mag=14.63 +/- 0.11 new_mean_mag=14.5981 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.73 +/- 0.12
Forced photometry filter REJECTED candidate at 22:52:06.25 +15:30:52.4: ref_mag=14.73 +/- 0.12 new_mean_mag=14.5755 delta=0.15 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:51:15.96 +15:23:31.1: 14.73 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.10
Forced photometry filter REJECTED candidate at 22:51:15.96 +15:23:31.1: ref_mag=14.66 +/- 0.10 new_mean_mag=14.5480 delta=0.11 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:48:38.53 +14:13:10.2: 14.95 +/- 0.19 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:52:21.87 +09:56:22.4: 14.94 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.14
Forced photometry filter REJECTED candidate at 22:48:38.53 +14:13:10.2: ref_mag=14.94 +/- 0.14 new_mean_mag=14.6140 delta=0.33 (need > 0.90)
Forced photometry reference-image weighted average: 14.91 +/- 0.13
Forced photometry filter REJECTED candidate at 22:52:21.87 +09:56:22.4: ref_mag=14.91 +/- 0.13 new_mean_mag=14.5928 delta=0.32 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:49:01.04 +14:10:30.9: 14.85 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.13
Forced photometry filter REJECTED candidate at 22:49:01.04 +14:10:30.9: ref_mag=14.90 +/- 0.13 new_mean_mag=14.5404 delta=0.35 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:49:30.87 +10:55:28.9: 15.31 +/- 0.28 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:48:48.71 +12:11:57.1: 14.76 +/- 0.16 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:52:39.81 +15:57:56.3: 14.77 +/- 0.15 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:57:19.35 +11:57:51.2: 14.89 +/- 0.18 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:52:59.60 +10:43:39.0: 15.13 +/- 0.23 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:01:27.15 +11:41:50.9: 14.79 +/- 0.16 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:54:39.21 +10:08:59.0: 15.05 +/- 0.21 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:03:42.23 +18:15:35.7: 14.60 +/- 0.13 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:49:30.87 +10:55:28.9: 14.97 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.17
Forced photometry filter REJECTED candidate at 22:49:30.87 +10:55:28.9: ref_mag=15.10 +/- 0.17 new_mean_mag=14.6818 delta=0.41 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:48:48.71 +12:11:57.1: 14.83 +/- 0.17 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:52:39.81 +15:57:56.3: 14.50 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.09
Forced photometry reference-image weighted average: 14.79 +/- 0.12
Forced photometry filter REJECTED candidate at 22:52:39.81 +15:57:56.3: ref_mag=14.60 +/- 0.09 new_mean_mag=14.5902 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:48:48.71 +12:11:57.1: ref_mag=14.79 +/- 0.12 new_mean_mag=14.7104 delta=0.08 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:57:19.35 +11:57:51.2: 14.97 +/- 0.18 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:52:59.60 +10:43:39.0: 15.05 +/- 0.22 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 22:57:50.75 +11:55:31.1: 14.62 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.13
Forced photometry filter REJECTED candidate at 22:57:19.35 +11:57:51.2: ref_mag=14.93 +/- 0.13 new_mean_mag=14.6666 delta=0.26 (need > 0.90)
Forced photometry reference-image weighted average: 15.09 +/- 0.16
Forced photometry filter REJECTED candidate at 22:52:59.60 +10:43:39.0: ref_mag=15.09 +/- 0.16 new_mean_mag=14.6120 delta=0.48 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:54:39.21 +10:08:59.0: 15.30 +/- 0.26 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:03:42.23 +18:15:35.7: 14.61 +/- 0.13 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:01:27.15 +11:41:50.9: 14.82 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.16
Forced photometry reference-image weighted average: 14.61 +/- 0.09
Forced photometry filter REJECTED candidate at 22:54:39.21 +10:08:59.0: ref_mag=15.15 +/- 0.16 new_mean_mag=14.7496 delta=0.40 (need > 0.90)
Forced photometry reference-image weighted average: 14.80 +/- 0.12
Forced photometry filter REJECTED candidate at 23:03:42.23 +18:15:35.7: ref_mag=14.61 +/- 0.09 new_mean_mag=14.6433 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:01:27.15 +11:41:50.9: ref_mag=14.80 +/- 0.12 new_mean_mag=14.6678 delta=0.14 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 22:57:50.75 +11:55:31.1: 14.65 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.10
Forced photometry filter REJECTED candidate at 22:57:50.75 +11:55:31.1: ref_mag=14.63 +/- 0.10 new_mean_mag=14.5391 delta=0.09 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:15:46.00 +16:17:50.4: 14.51 +/- 0.11 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:20:12.52 +17:42:47.3: 15.05 +/- 0.19 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-32-53_20.00sec_-15.00C_LIGHT_0070.fits at 23:20:07.08 +16:04:05.9: 12.40 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:20:07.08 +16:04:05.9: 12.45 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:15:46.00 +16:17:50.4: 14.57 +/- 0.12 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-01-20_20-33-41_20.00sec_-15.00C_LIGHT_0071.fits at 23:20:12.52 +17:42:47.3: 15.42 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.08
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter REJECTED candidate at 23:15:46.00 +16:17:50.4: ref_mag=14.54 +/- 0.08 new_mean_mag=14.6327 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 15.17 +/- 0.16
Forced photometry filter KEPT candidate at 23:20:07.08 +16:04:05.9: ref_mag=12.42 +/- 0.01 new_mean_mag=11.4694 delta=0.95 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:20:12.52 +17:42:47.3: ref_mag=15.17 +/- 0.16 new_mean_mag=14.7255 delta=0.45 (need > 0.90)
Adding exclusion_list_local.txt__out14445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60205.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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
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Considering the candidate 52622_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 52622_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 52624_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 52624_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 52626_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 52626_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 52627_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 52627_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 52628_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 52628_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 52635_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 52635_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 58655_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 58655_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 59319_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 59319_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 59491_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 59491_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 59704_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 59704_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 59883_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 59883_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 59896_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 59896_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60179_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60179_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 22:53:02.65 +16:48:20.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 60205_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 60205_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 60236_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60236_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60341_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60341_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60357_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60357_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60375_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60375_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60445_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60445_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60471_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60471_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60560_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60560_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60662_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60662_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60674_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60674_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60675_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60675_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60702_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60702_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60741_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60741_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60750_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60750_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60780_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60780_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60784_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60784_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60799_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60799_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60819_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60819_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60861_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60861_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60865_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60865_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 60884_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 60884_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61002_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61002_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61075_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61075_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61107_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61107_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61124_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61124_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61133_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61133_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61193_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61193_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61334_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61334_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61351_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61351_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61374_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61374_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61388_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61388_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61446_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61446_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61459_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61459_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61484_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61484_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61527_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61527_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61867_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61867_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 61979_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 61979_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 18036_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 18036_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 23:04:11.48 +15:18:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14445_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 14445_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 33951_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343
The candidate 33951_fd_Peg-10-Q2b1x1_2026-06-18_03-44-29_20.00sec_5.00C_LIGHT_0343 did not pass the final checks