This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 07.3819 2461167.8819 12.68 12:28:37.09 +15:15:16.9
277.70691 76.99521 galactic Com Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.402 Chloe -0 0 1 12.9 0 0
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits at 12:28:37.09 +15:15:16.9: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits at 12:28:37.09 +15:15:16.9: 16.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 07.3819* 12 28 37.09 +15 15 16.9 12.7 U Com 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461167.8819,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260507.3819 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 07.3819 2461167.8819 13.09 12:30:58.09 +12:18:31.1
283.99494 74.42289 galactic Vir Second-epoch detections are separated by 1.3" and 3.8 pix
The object was found in VSX 0" CV Vir
Type: M
# Max. Min./Amp. JD0 Period
12.500 V < 14.600 V 2453885.00000 149.300000000000 Me
The object was not found in astcheck.
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits at 12:30:58.09 +12:18:31.1: 14.04 +/- 0.05 detection
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits at 12:30:58.09 +12:18:31.1: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 07.3819* 12 30 58.09 +12 18 31.1 13.1 U Vir 9 0
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
CV Vir,2461167.8819,13.09,0.05,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
CV Vir 20260507.3819 13.09CV 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: 2461146.76060444 16.04.2026 06:15:06.224 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
First image: 2461146.76060444 16.04.2026 06:15:06.224 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
Last image: 2461167.88219590 07.05.2026 09:10:11.726 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.48
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: 3 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): 4270
Objects passed selection criteria: 4252
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 3309
Average stars matched: 3251.75 (98.2699 %)
Memory usage VmPeak: 110844 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 6 12:14:36 CDT 2026
VaST build number 1.0rc89-43-g0c21e0c3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 7 04:17:22 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: 2461146.76060444 16.04.2026 06:15:06.224 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
First image: 2461146.76060444 16.04.2026 06:15:06.224 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
Last image: 2461167.88219590 07.05.2026 09:10:11.726 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 106
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
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: 8 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): 21039
Objects passed selection criteria: 20997
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 16908
Average stars matched: 16370.2 (96.8196 %)
Memory usage VmPeak: 126884 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 6 12:14:36 CDT 2026
VaST build number 1.0rc89-43-g0c21e0c3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 7 04:18:52 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/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
SExtractor catalog cache: saved Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat to cache
SExtractor catalog cache: saved Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.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/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.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: 2461167.88165635
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits exists and is non-empty
Saving wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits to local_wcs_cache/
'wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits' -> 'local_wcs_cache/wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits'
wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits exists and is non-empty
Saving wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits to local_wcs_cache/
'wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits' -> 'local_wcs_cache/wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits'
wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits exists and is non-empty
Saving wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits to local_wcs_cache/
'wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits' -> 'local_wcs_cache/wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits'
wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits exists and is non-empty
Saving wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits to local_wcs_cache/
'wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits (1st reference image)
verification OK: wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:26:37.988 +14:01:45.24 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits (1st new image)
verification OK: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
Image size: 938.2'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: 12:26:40.321 +13:59:47.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:26:37.988 +14:01:45.24
Second-epoch image center 12:26:40.321 +13:59:47.38
Angular distance between the image centers 0.0341 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits (2nd new image)
verification OK: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
Image size: 938.2'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: 12:26:41.524 +13:59:31.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:26:37.988 +14:01:45.24
Second-epoch image center 12:26:41.524 +13:59:31.83
Angular distance between the image centers 0.0397 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 12:26:40.321 +13:59:47.38
Second-epoch second image center 12:26:41.524 +13:59:31.83
Angular distance between the image centers 0.00651 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/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits &> /tmp/tmp.jENceGOv4G
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits &> /tmp/tmp.szw3d2h5TE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits &> /tmp/tmp.yoqNhgqatj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits &> /tmp/tmp.h7F0fGXmur
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
Calibrating the magnitude scale
Found non-empty wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.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_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits and wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.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_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits and wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat
Found non-empty wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits and wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat
The reference image (wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits) and catalog (wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat) found
'wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat' -> 'wcsmag.cat'
Read 5830 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.3874 to 194.7978 deg, Dec +8.5979 to +19.3023 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 178.3874 to 194.7978 deg, Dec 8.5979 to 19.3023 deg
Loaded 3653 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): 2950 out of 3031 total matches.
Matched with Tycho-2 3031 out of 5830 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.844850
a=0.000000 b=1.000000 c=22.844850
From vast_summary.log: estimated ref. image limiting mag.: -7.48
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5830 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.3874 to 194.7978 deg, Dec +8.5979 to +19.3023 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 178.3874 to 194.7978 deg, Dec 8.5979 to 19.3023 deg
Loaded 3653 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): 2950 out of 3031 total matches.
Matched with Tycho-2 3031 out of 5830 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits:
Forced-photometry filter: calibrated wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits -> calib.txt_param_ref_wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits (aperture=6.4)
Read 5802 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.3876 to 194.7984 deg, Dec +8.5977 to +19.3023 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 178.3876 to 194.7984 deg, Dec 8.5977 to 19.3023 deg
Loaded 3654 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): 2936 out of 3033 total matches.
Matched with Tycho-2 3033 out of 5802 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits:
Forced-photometry filter: calibrated wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits -> calib.txt_param_ref_wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
2.4 pix Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
2.5 pix fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
2.5 pix fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
2.4 pix wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
2.4 pix wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
Limiting magnitude estimates:
15.4 mag. Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
15.4 mag. Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
13.9 mag. fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
14.0 mag. fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.4 (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.jENceGOv4G (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits' -> 'wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
Checking if the catalog wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
WCS catalog name: wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=307, passed=5830
Got 5830 stars (including 5519 good ones) from the SExtractor catalog wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 5830 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 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(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5764 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 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(), 5763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits -region wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.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.szw3d2h5TE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits' -> 'wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
WCS_IMAGE_NAME=wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
WCS-calibrated image found: wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
Checking if the catalog wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits alredy exist and is non-empty...
Catalog wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
WCS catalog name: wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=324, passed=5802
Got 5802 stars (including 5474 good ones) from the SExtractor catalog wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat
util/solve_plate_with_UCAC5 got 5802 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 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(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 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(), 5731 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5731 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits -region wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.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.yoqNhgqatj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
Checking if the catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
WCS catalog name: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=184, passed=2524
Got 2524 stars (including 2335 good ones) from the SExtractor catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 2524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 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(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 2465 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
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: 975 matched stars entering correct_measured_positions(), 2463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 2463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 975 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_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits -region wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.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.h7F0fGXmur (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
Checking if the catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
WCS catalog name: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=184, passed=2522
Got 2522 stars (including 2335 good ones) from the SExtractor catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 2522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 2463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 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(), 2465 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 2465 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 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_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits -region wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.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_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits'
Saving fully-calibrated image wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits'
Preparing the HTML report for the field Com-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Com-04-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/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
SExtractor catalog cache: saved Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat to cache
SExtractor catalog cache: saved Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
Creating symlink local_wcs_cache/wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
Creating symlink local_wcs_cache/wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
Creating symlink local_wcs_cache/wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.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_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits exists and is non-empty
wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits exists and is non-empty
wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits exists and is non-empty
wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits (1st reference image)
verification OK: wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:26:37.988 +14:01:45.24 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits (1st new image)
verification OK: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
Image size: 938.2'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: 12:26:40.321 +13:59:47.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:26:37.988 +14:01:45.24
Second-epoch image center 12:26:40.321 +13:59:47.38
Angular distance between the image centers 0.0341 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits (2nd new image)
verification OK: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
Image size: 938.2'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: 12:26:41.524 +13:59:31.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:26:37.988 +14:01:45.24
Second-epoch image center 12:26:41.524 +13:59:31.83
Angular distance between the image centers 0.0397 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 12:26:40.321 +13:59:47.38
Second-epoch second image center 12:26:41.524 +13:59:31.83
Angular distance between the image centers 0.00651 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/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits &> /tmp/tmp.zD8C6XlXCi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits &> /tmp/tmp.0Rkam56Thn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits &> /tmp/tmp.sHI75mMHrp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits &> /tmp/tmp.ykccekkdQ7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
Calibrating the magnitude scale
Found non-empty wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.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_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits and wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.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_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits and wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat
Found non-empty wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits and wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat
The reference image (wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits) and catalog (wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat) found
'wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat' -> 'wcsmag.cat'
Read 27491 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.3327 to 194.8283 deg, Dec +8.5941 to +19.3139 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 178.3327 to 194.8283 deg, Dec 8.5941 to 19.3139 deg
Loaded 3676 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): 2855 out of 3044 total matches.
Matched with Tycho-2 3044 out of 27491 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.739300
a=0.000000 b=1.000000 c=22.739300
From vast_summary.log: estimated ref. image limiting mag.: -7.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.51
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27491 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.3327 to 194.8283 deg, Dec +8.5941 to +19.3139 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 178.3327 to 194.8283 deg, Dec 8.5941 to 19.3139 deg
Loaded 3676 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): 2855 out of 3044 total matches.
Matched with Tycho-2 3044 out of 27491 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits:
Forced-photometry filter: calibrated wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits -> calib.txt_param_ref_wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits (aperture=5.1)
Read 27838 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.3571 to 194.8466 deg, Dec +8.5977 to +19.3131 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 178.3571 to 194.8466 deg, Dec 8.5977 to 19.3131 deg
Loaded 3671 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): 2839 out of 3045 total matches.
Matched with Tycho-2 3045 out of 27838 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits:
Forced-photometry filter: calibrated wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits -> calib.txt_param_ref_wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 63 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
2.3 pix Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
2.5 pix fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
2.4 pix fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
2.3 pix wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
2.3 pix wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
Limiting magnitude estimates:
15.5 mag. Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
15.5 mag. Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
14.3 mag. fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
14.3 mag. fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zD8C6XlXCi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits' -> 'wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
Checking if the catalog wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits
WCS catalog name: wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1137, passed=27481
Got 27481 stars (including 26304 good ones) from the SExtractor catalog wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 27481 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 27166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 27163 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 27162 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits -region wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.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.0Rkam56Thn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits' -> 'wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
WCS_IMAGE_NAME=wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
WCS-calibrated image found: wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
Checking if the catalog wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits alredy exist and is non-empty...
Catalog wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits
WCS catalog name: wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1202, passed=27825
Got 27825 stars (including 26588 good ones) from the SExtractor catalog wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat
util/solve_plate_with_UCAC5 got 27825 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 27483 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 27480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 27479 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits -region wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.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.sHI75mMHrp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
Checking if the catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
WCS catalog name: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=597, passed=12722
Got 12722 stars (including 12105 good ones) from the SExtractor catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 12722 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 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(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 12375 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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 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(), 12378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 12378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits -region wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.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.ykccekkdQ7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
Checking if the catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
WCS catalog name: wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=564, passed=12691
Got 12691 stars (including 12099 good ones) from the SExtractor catalog wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 12691 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 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(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 12403 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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 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(), 12405 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 12405 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits -region wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.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_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/wcs_fd_Com-04-Q2b1x1_2026-05-07_04-09-25_20.00sec_-5.00C_LIGHT_0038.fits
Saving fully-calibrated image wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Com-04-Q2b1x1_041500_TTUQ2b1x1_1241219_gSVCIa7j/wcs_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039.fits
Preparing the HTML report for the field Com-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits at 12:38:28.19 +13:47:30.7: 12.17 +/- 0.01 detection
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits at 12:28:37.09 +15:15:16.9: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits at 12:55:06.87 +17:18:51.1: 12.79 +/- 0.02 detection
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits at 12:38:28.19 +13:47:30.7: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 12:38:28.19 +13:47:30.7: ref_mag=12.17 +/- 0.01 new_mean_mag=12.3377 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits at 12:55:06.87 +17:18:51.1: 12.85 +/- 0.02 detection
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits at 12:28:37.09 +15:15:16.9: 16.20 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter REJECTED candidate at 12:55:06.87 +17:18:51.1: ref_mag=12.81 +/- 0.02 new_mean_mag=13.1691 delta=-0.35 (need > 0.90)
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits at 12:26:08.08 +13:06:46.0: 13.74 +/- 0.04 detection
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits at 12:26:08.08 +13:06:46.0: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter REJECTED candidate at 12:26:08.08 +13:06:46.0: ref_mag=13.73 +/- 0.03 new_mean_mag=13.4625 delta=0.27 (need > 0.90)
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-15-06_20.00sec_-5.00C_LIGHT_0222.fits at 12:30:58.09 +12:18:31.1: 14.04 +/- 0.05 detection
Forced photometry on wcs_Com-04-Q2b1x1_2026-04-16_01-16-01_20.00sec_-4.90C_LIGHT_0223.fits at 12:30:58.09 +12:18:31.1: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.04
Forced photometry filter KEPT candidate at 12:30:58.09 +12:18:31.1: ref_mag=14.07 +/- 0.04 new_mean_mag=13.0830 delta=0.98 (need > 0.90)
Adding exclusion_list_local.txt__out26787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31972.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 31922_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31922_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
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Considering the candidate 31929_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31929_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 31938_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31938_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 31939_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31939_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 31945_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31945_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 31950_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31950_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 31952_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31952_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 31960_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31960_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 31962_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31962_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 31963_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31963_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 31966_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31966_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 31969_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31969_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 31971_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31971_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 31972_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
Preparing report for the candidate 31972_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
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Considering the candidate 31973_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31973_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 31974_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31974_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 31982_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31982_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
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Considering the candidate 31984_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31984_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 31987_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31987_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 31988_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31988_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 31992_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31992_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 31995_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31995_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 31997_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 31997_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 32000_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32000_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 32001_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32001_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 32003_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32003_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 32004_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32004_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 32005_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32005_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 32006_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32006_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 32007_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32007_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 32010_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32010_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 32011_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32011_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 32013_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32013_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 32014_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32014_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 32019_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32019_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 32021_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32021_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 32026_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32026_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 32027_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32027_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 32028_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32028_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 32031_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32031_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 32032_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32032_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 32033_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32033_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 32035_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32035_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 32036_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32036_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 32042_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32042_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 32043_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32043_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 32044_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32044_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 32049_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32049_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
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Considering the candidate 32050_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32050_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 32051_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32051_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 32057_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32057_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 32065_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32065_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 32067_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32067_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 32070_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32070_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 32074_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32074_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 32077_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32077_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 32079_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32079_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 32080_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32080_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 32082_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32082_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 32084_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32084_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 32088_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32088_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 32094_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039
The candidate 32094_fd_Com-04-Q2b1x1_2026-05-07_04-10-11_20.00sec_-4.90C_LIGHT_0039 did not pass the final checks