This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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
ASASSN-V J231602.13+331341.1,2461149.9479,12.79,0.05,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
ASASSN-V J231602.13+331341.1 20260419.4479 12.79CV 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
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
NSVS J2312245+281700,2461149.9479,11.86,0.05,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
NSVS J2312245+281700 20260419.4479 11.86CV 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: 2461036.56213631 27.12.2025 01:29:18.577 /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
First image: 2461036.56213631 27.12.2025 01:29:18.577 /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
Last image: 2461149.94816375 19.04.2026 10:45:11.348 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.88
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: 5 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): 11547
Objects passed selection criteria: 11498
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 8380.75
Average stars matched: 7505.25 (89.5534 %)
Memory usage VmPeak: 115472 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 05:51:13 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: 2461036.56213631 27.12.2025 01:29:18.577 /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
First image: 2461036.56213631 27.12.2025 01:29:18.577 /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
Last image: 2461149.94816375 19.04.2026 10:45:11.348 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 42
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
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: 48 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): 70567
Objects passed selection criteria: 70369
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 51883
Average stars matched: 46521.8 (89.6667 %)
Memory usage VmPeak: 163256 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 05:53:23 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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
SExtractor catalog cache: saved Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat to cache
SExtractor catalog cache: saved Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.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: 2461149.94754008
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits exists and is non-empty
Saving wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits to local_wcs_cache/
'wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits' -> 'local_wcs_cache/wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits'
wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits exists and is non-empty
Saving wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits to local_wcs_cache/
'wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits' -> 'local_wcs_cache/wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits'
wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits exists and is non-empty
Saving wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits to local_wcs_cache/
'wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits' -> 'local_wcs_cache/wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits'
wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits exists and is non-empty
Saving wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits to local_wcs_cache/
'wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits' -> 'local_wcs_cache/wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits (1st reference image)
verification OK: wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:00:01.010 +29:59:55.94 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-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits (1st new image)
verification OK: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
Image size: 938.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:59:40.825 +30:01:30.88 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:00:01.010 +29:59:55.94
Second-epoch image center 22:59:40.825 +30:01:30.88
Angular distance between the image centers 0.0775 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits (2nd new image)
verification OK: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
Image size: 938.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:59:43.963 +30:02:08.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:00:01.010 +29:59:55.94
Second-epoch image center 22:59:43.963 +30:02:08.78
Angular distance between the image centers 0.0717 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:59:40.825 +30:01:30.88
Second-epoch second image center 22:59:43.963 +30:02:08.78
Angular distance between the image centers 0.01546 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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits &> /tmp/tmp.q9O9PkicAd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits &> /tmp/tmp.FtL1crhNo9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits &> /tmp/tmp.JPsU1cnD3K
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits &> /tmp/tmp.8UegFmBOTX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits and wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits and wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat
Found non-empty wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits and wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat
The reference image (wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits) and catalog (wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat) found
'wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat' -> 'wcsmag.cat'
Read 12930 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 335.5798 to 354.6894 deg, Dec +24.3435 to +35.3134 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 335.5798 to 354.6894 deg, Dec 24.3435 to 35.3134 deg
Loaded 11370 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): 8173 out of 8678 total matches.
Matched with Tycho-2 8678 out of 12930 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.943140
a=0.000000 b=1.000000 c=22.943140
From vast_summary.log: estimated ref. image limiting mag.: -7.88
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.06
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.06
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
2.5 pix Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
2.9 pix fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
2.9 pix fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
Limiting magnitude estimates:
15.1 mag. Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
15.1 mag. Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
14.3 mag. fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
14.3 mag. fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.7 (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.q9O9PkicAd (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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits' -> 'wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
WCS_IMAGE_NAME=wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
WCS-calibrated image found: wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
Checking if the catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat corresponding to the image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits alredy exist and is non-empty...
Catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat corresponding to the image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
WCS catalog name: wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1041, passed=12928
Got 12928 stars (including 11871 good ones) from the SExtractor catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat
util/solve_plate_with_UCAC5 got 12928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 12624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 12622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 12622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits -region wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FtL1crhNo9 (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-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.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-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.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-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits' -> 'wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
WCS-calibrated image found: wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
Checking if the catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
WCS catalog name: wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1039, passed=12956
Got 12956 stars (including 11903 good ones) from the SExtractor catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 12956 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 975 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(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 12704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 975 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(), 12704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 12704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits -region wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JPsU1cnD3K (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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
WCS_IMAGE_NAME=wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
WCS-calibrated image found: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
Checking if the catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat corresponding to the image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat corresponding to the image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
WCS catalog name: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=606, passed=8741
Got 8741 stars (including 8129 good ones) from the SExtractor catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat
util/solve_plate_with_UCAC5 got 8741 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 8512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 8511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 8511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits -region wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8UegFmBOTX (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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
WCS_IMAGE_NAME=wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
WCS-calibrated image found: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
Checking if the catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat corresponding to the image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat corresponding to the image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
WCS catalog name: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=640, passed=8766
Got 8766 stars (including 8121 good ones) from the SExtractor catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat
util/solve_plate_with_UCAC5 got 8766 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8510 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8510 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits -region wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits'
Saving fully-calibrated image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits'
Saving fully-calibrated image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits'
Saving fully-calibrated image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits'
Preparing the HTML report for the field Peg-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20776_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 20776_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:52:18.15 +34:13:33.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21818_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 21818_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:07:48.10 +29:17:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10960_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 10960_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:19:50.04 +26:16:47.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Peg-03-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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
SExtractor catalog cache: saved Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat to cache
SExtractor catalog cache: saved Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
Creating symlink local_wcs_cache/wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits exists and is non-empty
wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits exists and is non-empty
wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits exists and is non-empty
wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits (1st reference image)
verification OK: wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:00:01.010 +29:59:55.94 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-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits (1st new image)
verification OK: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
Image size: 938.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:59:40.825 +30:01:30.88 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:00:01.010 +29:59:55.94
Second-epoch image center 22:59:40.825 +30:01:30.88
Angular distance between the image centers 0.0775 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits (2nd new image)
verification OK: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
Image size: 938.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:59:43.963 +30:02:08.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:00:01.010 +29:59:55.94
Second-epoch image center 22:59:43.963 +30:02:08.78
Angular distance between the image centers 0.0717 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:59:40.825 +30:01:30.88
Second-epoch second image center 22:59:43.963 +30:02:08.78
Angular distance between the image centers 0.01546 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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits &> /tmp/tmp.X0zHgvkMer
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits &> /tmp/tmp.vRSBvf9jRl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits &> /tmp/tmp.l8mncQy4cE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits &> /tmp/tmp.WwZzES9P2j
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits and wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits and wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat
Found non-empty wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits and wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat
The reference image (wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits) and catalog (wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat) found
'wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat' -> 'wcsmag.cat'
Read 82089 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 335.5798 to 354.6894 deg, Dec +24.3150 to +35.3134 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 335.5798 to 354.6894 deg, Dec 24.3150 to 35.3134 deg
Loaded 11386 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): 7563 out of 9088 total matches.
Matched with Tycho-2 9088 out of 82089 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.773334
a=0.000000 b=1.000000 c=22.773334
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
2.2 pix Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
2.8 pix fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
2.8 pix fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
Limiting magnitude estimates:
15.2 mag. Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
15.2 mag. Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
14.5 mag. fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
14.5 mag. fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 13.9 (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.X0zHgvkMer (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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.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-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits' -> 'wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
WCS_IMAGE_NAME=wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
WCS-calibrated image found: wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
Checking if the catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat corresponding to the image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits alredy exist and is non-empty...
Catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat corresponding to the image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
WCS catalog name: wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=6201, passed=82059
Got 82059 stars (including 75724 good ones) from the SExtractor catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat
util/solve_plate_with_UCAC5 got 82059 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 975 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(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 80447 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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 975 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(), 80447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 80448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits -region wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.vRSBvf9jRl (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-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.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-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.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-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits' -> 'wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
WCS-calibrated image found: wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
Checking if the catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
WCS catalog name: wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=6132, passed=82163
Got 82163 stars (including 75899 good ones) from the SExtractor catalog wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 82163 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 80920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 80919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 80919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits -region wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.l8mncQy4cE (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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
WCS_IMAGE_NAME=wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
WCS-calibrated image found: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
Checking if the catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat corresponding to the image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat corresponding to the image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
WCS catalog name: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=3804, passed=46995
Got 46995 stars (including 43137 good ones) from the SExtractor catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat
util/solve_plate_with_UCAC5 got 46995 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 976 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(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 45786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 976 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(), 45786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 45786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits -region wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WwZzES9P2j (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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
WCS_IMAGE_NAME=wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
WCS-calibrated image found: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
Checking if the catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat corresponding to the image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat corresponding to the image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
WCS catalog name: wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=3767, passed=47565
Got 47565 stars (including 43748 good ones) from the SExtractor catalog wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat
util/solve_plate_with_UCAC5 got 47565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 45860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 45863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 45863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits -region wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/wcs_Peg-03-Q2b1x1_2025-12-26_19-29-18_20.00sec_-15.00C_LIGHT_0030.fits
Saving fully-calibrated image wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/wcs_Peg-03-Q2b1x1_2025-12-26_19-29-58_20.00sec_-15.00C_LIGHT_0031.fits
Saving fully-calibrated image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-44-17_20.00sec_-4.90C_LIGHT_0752.fits
Saving fully-calibrated image wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.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_2026-04-19_CI_Peg-03-Q2b1x1_054550_TTUQ2b1x1_3796771_MtRIZhcN/wcs_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753.fits
Preparing the HTML report for the field Peg-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out111552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out97119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out97122.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out16626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80610.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 42s
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: 2s
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Considering the candidate 97119_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 97119_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:17:08.95 +30:43:29.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 97122_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 97122_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:54:01.04 +34:04:19.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)
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Considering the candidate 97125_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 97125_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:09:26.64 +32:12:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97743_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 97743_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:04:04.36 +28:04:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98647_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 98647_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:07:48.09 +29:17:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99873_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 99873_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:49:21.56 +32:32:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102106_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 102106_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:51:39.53 +32:49:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102142_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 102142_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:56:44.35 +34:12:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103010_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 103010_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:41:35.21 +33:28:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103217_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 103217_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:07:47.76 +30:24:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103620_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 103620_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:47:50.33 +30:07:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104347_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 104347_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:51:32.78 +26:23:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104384_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 104384_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:00:03.91 +28:58:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104449_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 104449_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:18:31.82 +27:35:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104461_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 104461_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:09:14.11 +26:56:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104669_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 104669_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:49:37.04 +31:18:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104727_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 104727_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:59:47.56 +33:46:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105083_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 105083_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:39:52.52 +32:31:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105178_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 105178_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:17:36.68 +33:15:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106734_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 106734_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:55:30.96 +34:08:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106918_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 106918_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:03:21.96 +33:08:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107458_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 107458_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:42:58.09 +33:32:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107503_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 107503_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:58:54.89 +34:03:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107743_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 107743_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:11:58.31 +32:26:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108712_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 108712_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:08:24.64 +30:32:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108838_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 108838_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:41:50.53 +30:02:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108922_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 108922_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:48:24.37 +28:07:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109281_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 109281_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:48:19.05 +33:49:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110480_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 110480_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:40:23.76 +31:19:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111401_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 111401_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:48:56.76 +33:41:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111552_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 111552_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 22:44:29.02 +32:51:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.671 1890726487253491200 341.12092576428 +32.85881379841 14.4729 13.9805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 63692_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 63692_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks
**** FOUND 23:19:50.07 +26:16:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92395_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753
The candidate 92395_fd_Peg-03-Q2b1x1_2026-04-19_05-45-11_20.00sec_-4.90C_LIGHT_0753 did not pass the final checks