This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB
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 03.4376 2461163.9376 12.87 15:29:30.63 +05:59:33.5
10.83604 46.92083 galactic Ser Second-epoch detections are separated by 1.8" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.472 Roma 0 -1 1 13.0 -0 0
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:29:30.63 +05:59:33.5: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:29:30.63 +05:59:33.5: 16.24 +/- 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 03.4376* 15 29 30.63 +05 59 33.5 12.9 U Ser 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,2461163.9376,12.87,0.05,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 20260503.4376 12.87CV 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 03.4376 2461163.9376 13.06 15:28:39.21 +05:00:49.9
9.48264 46.54265 galactic Ser Second-epoch detections are separated by 1.0" and 3.6 pix
The object was found in VSX 1" V0443 Ser
Type: RRAB
# Max. Min./Amp. JD0 Period
12.900 V 14.300 V 2453909.67000 0.535286000000
The object was not found in astcheck.
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:28:39.21 +05:00:49.9: 14.09 +/- 0.05 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:28:39.21 +05:00:49.9: 14.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.08 +/- 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 03.4376* 15 28 39.21 +05 00 49.9 13.1 U Ser 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
V0443 Ser,2461163.9376,13.06,0.05,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
V0443 Ser 20260503.4376 13.06CV 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: 2461120.98298340 21.03.2026 11:35:19.766 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
First image: 2461120.98298340 21.03.2026 11:35:19.766 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Last image: 2461163.93785582 03.05.2026 10:30:20.743 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.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.: -7.63
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): 6601
Objects passed selection criteria: 6576
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 4816.25
Average stars matched: 4738.25 (98.3805 %)
Memory usage VmPeak: 113112 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 05:32:32 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: 2461120.98298340 21.03.2026 11:35:19.766 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
First image: 2461120.98298340 21.03.2026 11:35:19.766 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Last image: 2461163.93785582 03.05.2026 10:30:20.743 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 37
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
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): 39235
Objects passed selection criteria: 39144
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 30099.2
Average stars matched: 28955.8 (96.2009 %)
Memory usage VmPeak: 144200 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 05:33:48 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/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat to cache
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.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/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.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: 2461163.93733336
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits exists and is non-empty
Saving wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits to local_wcs_cache/
'wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits' -> 'local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits'
wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits exists and is non-empty
Saving wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits to local_wcs_cache/
'wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits' -> 'local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits'
wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits exists and is non-empty
Saving wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits to local_wcs_cache/
'wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits' -> 'local_wcs_cache/wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits'
wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits exists and is non-empty
Saving wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits to local_wcs_cache/
'wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits' -> 'local_wcs_cache/wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits (1st reference image)
verification OK: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Image size: 937.4'x624.3' 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: 15:25:45.434 +05:59:44.20 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_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits (1st new image)
verification OK: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:24.456 +06:01:24.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:45.434 +05:59:44.20
Second-epoch image center 15:25:24.456 +06:01:24.68
Angular distance between the image centers 0.0913 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits (2nd new image)
verification OK: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:25.915 +06:01:20.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:45.434 +05:59:44.20
Second-epoch image center 15:25:25.915 +06:01:20.40
Angular distance between the image centers 0.0852 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 15:25:24.456 +06:01:24.68
Second-epoch second image center 15:25:25.915 +06:01:20.40
Angular distance between the image centers 0.00616 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/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits &> /tmp/tmp.oG1v49eqOt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits &> /tmp/tmp.EAgdXh9CKG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits &> /tmp/tmp.hT2XaaCyxI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits &> /tmp/tmp.GIXEaDEsLZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.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_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.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_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
Found non-empty wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
The reference image (wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits) and catalog (wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat) found
'wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat' -> 'wcsmag.cat'
Read 8926 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5451 to 239.4424 deg, Dec +0.6561 to +11.2816 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 223.5451 to 239.4424 deg, Dec 0.6561 to 11.2816 deg
Loaded 4656 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): 3898 out of 4076 total matches.
Matched with Tycho-2 4076 out of 8926 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.928400
a=0.000000 b=1.000000 c=22.928400
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8926 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5451 to 239.4424 deg, Dec +0.6561 to +11.2816 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 223.5451 to 239.4424 deg, Dec 0.6561 to 11.2816 deg
Loaded 4656 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): 3898 out of 4076 total matches.
Matched with Tycho-2 4076 out of 8926 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits (aperture=6.4)
Read 8697 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5431 to 239.4424 deg, Dec +0.6252 to +11.2700 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 223.5431 to 239.4424 deg, Dec 0.6252 to 11.2700 deg
Loaded 4669 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): 3846 out of 4063 total matches.
Matched with Tycho-2 4063 out of 8697 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits (aperture=6.2)
____ 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 Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
2.3 pix Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
2.4 pix fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
2.3 pix fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
2.4 pix wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
2.3 pix wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Limiting magnitude estimates:
15.3 mag. Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
15.3 mag. Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
14.0 mag. fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
14.0 mag. fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.2 (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.oG1v49eqOt (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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits' -> 'wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=521, passed=8926
Got 8926 stars (including 8397 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
util/solve_plate_with_UCAC5 got 8926 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
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(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8797 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 453 to 508 (Dec 0.7 to 11.3)
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(), 8798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8798 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_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits -region wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.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.EAgdXh9CKG (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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits' -> 'wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=573, passed=8695
Got 8695 stars (including 8117 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat
util/solve_plate_with_UCAC5 got 8695 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
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(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 8555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 8555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 8555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits -region wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.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.hT2XaaCyxI (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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
WCS_IMAGE_NAME=wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
WCS-calibrated image found: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
Checking if the catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
WCS catalog name: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=327, passed=3356
Got 3356 stars (including 3027 good ones) from the SExtractor catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat
util/solve_plate_with_UCAC5 got 3356 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 957 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(), 3299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
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: 974 matched stars entering correct_measured_positions(), 3299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 3299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits -region wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.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.GIXEaDEsLZ (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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
WCS_IMAGE_NAME=wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
WCS-calibrated image found: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
Checking if the catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
WCS catalog name: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=359, passed=3310
Got 3310 stars (including 2949 good ones) from the SExtractor catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat
util/solve_plate_with_UCAC5 got 3310 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 959 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(), 3247 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
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: 974 matched stars entering correct_measured_positions(), 3246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 3246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits -region wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.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_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits'
Saving fully-calibrated image wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits'
Preparing the HTML report for the field Ser-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ser-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat to cache
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Creating symlink local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.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_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits exists and is non-empty
wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits exists and is non-empty
wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits exists and is non-empty
wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits (1st reference image)
verification OK: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Image size: 937.4'x624.3' 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: 15:25:45.434 +05:59:44.20 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_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits (1st new image)
verification OK: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:24.456 +06:01:24.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:45.434 +05:59:44.20
Second-epoch image center 15:25:24.456 +06:01:24.68
Angular distance between the image centers 0.0913 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits (2nd new image)
verification OK: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:25.915 +06:01:20.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:45.434 +05:59:44.20
Second-epoch image center 15:25:25.915 +06:01:20.40
Angular distance between the image centers 0.0852 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 15:25:24.456 +06:01:24.68
Second-epoch second image center 15:25:25.915 +06:01:20.40
Angular distance between the image centers 0.00616 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/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits &> /tmp/tmp.yhlpOsAn7Z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits &> /tmp/tmp.9mAWpL07LR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits &> /tmp/tmp.6hyv2f1vy2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits &> /tmp/tmp.RTjM1YLZM7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.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_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.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_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
Found non-empty wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
The reference image (wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits) and catalog (wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat) found
'wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat' -> 'wcsmag.cat'
Read 50422 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5430 to 239.4714 deg, Dec +0.6305 to +11.2886 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 223.5430 to 239.4714 deg, Dec 0.6305 to 11.2886 deg
Loaded 4685 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): 3662 out of 4090 total matches.
Matched with Tycho-2 4090 out of 50422 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.812400
a=0.000000 b=1.000000 c=22.812400
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 50422 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5430 to 239.4714 deg, Dec +0.6305 to +11.2886 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 223.5430 to 239.4714 deg, Dec 0.6305 to 11.2886 deg
Loaded 4685 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): 3662 out of 4090 total matches.
Matched with Tycho-2 4090 out of 50422 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits (aperture=5.0)
Read 51564 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5411 to 239.4698 deg, Dec +0.6229 to +11.2765 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 223.5411 to 239.4698 deg, Dec 0.6229 to 11.2765 deg
Loaded 4682 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): 3631 out of 4069 total matches.
Matched with Tycho-2 4069 out of 51564 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 27 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
2.1 pix Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
2.4 pix fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
2.3 pix fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
2.3 pix wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
2.1 pix wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Limiting magnitude estimates:
15.5 mag. Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
15.5 mag. Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
14.2 mag. fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
14.2 mag. fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.6 (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.yhlpOsAn7Z (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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits' -> 'wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2486, passed=50406
Got 50406 stars (including 47846 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
util/solve_plate_with_UCAC5 got 50406 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 49664 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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 49665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 49664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits -region wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.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.9mAWpL07LR (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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits' -> 'wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2509, passed=51546
Got 51546 stars (including 48975 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat
util/solve_plate_with_UCAC5 got 51546 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 50857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
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(), 50857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 50856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits -region wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.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.6hyv2f1vy2 (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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
WCS_IMAGE_NAME=wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
WCS-calibrated image found: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
Checking if the catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
WCS catalog name: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=877, passed=19868
Got 19868 stars (including 18957 good ones) from the SExtractor catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat
util/solve_plate_with_UCAC5 got 19868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 19560 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 19559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 19559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits -region wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.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.RTjM1YLZM7 (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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
WCS_IMAGE_NAME=wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
WCS-calibrated image found: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
Checking if the catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
WCS catalog name: wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=948, passed=20232
Got 20232 stars (including 19259 good ones) from the SExtractor catalog wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat
util/solve_plate_with_UCAC5 got 20232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 19844 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 19844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 19844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits -region wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.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_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-29-35_20.00sec_-4.90C_LIGHT_0419.fits
Saving fully-calibrated image wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.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_2026-05-03_CI_Ser-03-Q2b1x1_053106_TTUQ2b1x1_4104700_IW00adwB/wcs_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420.fits
Preparing the HTML report for the field Ser-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:29:30.63 +05:59:33.5: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:29:30.63 +05:59:33.5: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:28:39.21 +05:00:49.9: 14.09 +/- 0.05 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:28:39.21 +05:00:49.9: 14.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.04
Forced photometry filter KEPT candidate at 15:28:39.21 +05:00:49.9: ref_mag=14.08 +/- 0.04 new_mean_mag=13.0628 delta=1.02 (need > 0.90)
Adding exclusion_list_local.txt__out29803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64808.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64651_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64651_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:34:52.86 +07:59:59.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64729_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64729_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64744_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64744_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:18:42.88 +02:07:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64757_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64757_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64763_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64763_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:18:39.58 +02:07:16.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64764_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64764_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64788_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64788_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:18:24.45 +02:02:00.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64792_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64792_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64803_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64803_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64808_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
Preparing report for the candidate 64808_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64809_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64809_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:18:45.70 +02:07:20.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64816_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64816_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:34:52.38 +06:49:06.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64821_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64821_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:50:22.46 +02:13:06.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64835_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64835_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:45:17.98 +05:25:37.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64856_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64856_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64858_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64858_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:44:08.41 +08:06:54.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64860_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64860_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64861_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64861_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:41:06.44 +09:16:44.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64873_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64873_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:26:47.96 +05:12:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64878_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64878_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:40:34.11 +06:51:17.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64884_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64884_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:44:06.54 +04:41:38.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64886_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64886_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64918_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64918_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64924_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64924_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:34:40.92 +04:40:34.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64931_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64931_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks
**** FOUND 15:42:25.42 +03:19:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64945_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420
The candidate 64945_fd_Ser-03-Q2b1x1_2026-05-03_05-30-20_20.00sec_-5.00C_LIGHT_0420 did not pass the final checks