This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI
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 18.1900 2461178.6900 12.73 12:59:33.85 -08:46:33.0
306.35251 54.04194 galactic Vir Second-epoch detections are separated by 0.3" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.233 Asterope 1 0 1 13.0 0 -0
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:59:33.85 -08:46:33.0: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:59:33.85 -08:46:33.0: 15.67 +/- 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 18.1900* 12 59 33.85 -08 46 33.0 12.7 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461178.6900,12.73,0.05,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 20260518.1900 12.73CV 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 18.1900 2461178.6900 12.68 12:49:20.32 -08:21:34.5
302.03755 54.50852 galactic Vir Second-epoch detections are separated by 0.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.55 Pandora 1 -0 1 12.9 0 -0
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:49:20.32 -08:21:34.5: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:49:20.32 -08:21:34.5: 15.73 +/- 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 18.1900* 12 49 20.32 -08 21 34.5 12.7 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461178.6900,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260518.1900 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 18.1900 2461178.6900 13.13 13:07:13.85 -06:10:04.5
310.05385 56.48529 galactic Vir Second-epoch detections are separated by 0.7" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.178 Belisana 0 -0 0 13.2 0 -0
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:07:13.85 -06:10:04.5: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:07:13.85 -06:10:04.5: 15.58 +/- 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 18.1900* 13 07 13.85 -06 10 04.5 13.1 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461178.6900,13.13,0.05,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 20260518.1900 13.13CV 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: 2461082.91602938 11.02.2026 09:58:54.938 /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
First image: 2461082.91602938 11.02.2026 09:58:54.938 /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
Last image: 2461178.69021848 18.05.2026 04:33:44.877 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.80
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): 4476
Objects passed selection criteria: 4476
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 4327.5
Average stars matched: 3902 (90.1675 %)
Memory usage VmPeak: 111204 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 17 23:40:01 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: 2461082.91602938 11.02.2026 09:58:54.938 /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
First image: 2461082.91602938 11.02.2026 09:58:54.938 /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
Last image: 2461178.69021848 18.05.2026 04:33:44.877 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 36
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
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: 9 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): 26195
Objects passed selection criteria: 26137
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 25766
Average stars matched: 23608.5 (91.6266 %)
Memory usage VmPeak: 132540 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 17 23:41:31 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/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
SExtractor catalog cache: saved Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat to cache
SExtractor catalog cache: saved Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.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/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.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: 2461178.68977738
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_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits exists and is non-empty
Saving wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits to local_wcs_cache/
'wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits' -> 'local_wcs_cache/wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits'
wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits exists and is non-empty
Saving wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits to local_wcs_cache/
'wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits' -> 'local_wcs_cache/wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits'
wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits exists and is non-empty
Saving wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits to local_wcs_cache/
'wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits' -> 'local_wcs_cache/wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits'
wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits exists and is non-empty
Saving wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits to local_wcs_cache/
'wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits' -> 'local_wcs_cache/wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits (1st reference image)
verification OK: wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
Image size: 941.6'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:51:17.659 -09:58:37.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits (1st new image)
verification OK: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 936.8'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:51:26.385 -09:59:49.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:51:17.659 -09:58:37.31
Second-epoch image center 12:51:26.385 -09:59:49.21
Angular distance between the image centers 0.0410 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits (2nd new image)
verification OK: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
Image size: 936.8'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:51:26.014 -09:59:35.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:51:17.659 -09:58:37.31
Second-epoch image center 12:51:26.014 -09:59:35.01
Angular distance between the image centers 0.0378 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:51:26.385 -09:59:49.21
Second-epoch second image center 12:51:26.014 -09:59:35.01
Angular distance between the image centers 0.00423 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/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits &> /tmp/tmp.t30KoDgU2S
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits &> /tmp/tmp.SRN1xUZdTQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits &> /tmp/tmp.gdRe6CY55L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits &> /tmp/tmp.vaNulC9byr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.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_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits and wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.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_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits and wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat
Found non-empty wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits and wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat
The reference image (wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits) and catalog (wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat) found
'wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat' -> 'wcsmag.cat'
Read 5760 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 184.7361 to 200.9220 deg, Dec -15.2510 to -4.6700 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 184.7361 to 200.9220 deg, Dec -15.2510 to -4.6700 deg
Loaded 4165 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): 3283 out of 3467 total matches.
Matched with Tycho-2 3467 out of 5760 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.873200
a=0.000000 b=1.000000 c=22.873200
From vast_summary.log: estimated ref. image limiting mag.: -7.80
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5760 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 184.7361 to 200.9220 deg, Dec -15.2510 to -4.6700 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 184.7361 to 200.9220 deg, Dec -15.2510 to -4.6700 deg
Loaded 4165 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): 3283 out of 3467 total matches.
Matched with Tycho-2 3467 out of 5760 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits:
Forced-photometry filter: calibrated wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits -> calib.txt_param_ref_wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits (aperture=6.0)
Read 5181 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 184.8992 to 201.0615 deg, Dec -15.3017 to -4.6477 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 184.8992 to 201.0615 deg, Dec -15.3017 to -4.6477 deg
Loaded 4171 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): 3241 out of 3339 total matches.
Matched with Tycho-2 3339 out of 5181 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits:
Forced-photometry filter: calibrated wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits -> calib.txt_param_ref_wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
2.3 pix Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
2.6 pix fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
2.6 pix fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
2.1 pix wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
2.3 pix wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
Limiting magnitude estimates:
15.1 mag. Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
14.8 mag. Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
14.9 mag. fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
14.9 mag. fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.t30KoDgU2S (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits' -> 'wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
WCS_IMAGE_NAME=wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
WCS-calibrated image found: wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
Checking if the catalog wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat corresponding to the image wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits alredy exist and is non-empty...
Catalog wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat corresponding to the image wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
WCS catalog name: wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=475, passed=5760
Got 5760 stars (including 5278 good ones) from the SExtractor catalog wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat
util/solve_plate_with_UCAC5 got 5760 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 5685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 5685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 5685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits N_match=980 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.454 sigma_q2_arcsec=0.336 sigma_q3_arcsec=0.356 sigma_q4_arcsec=0.342 n_q1=213 n_q2=271 n_q3=248 n_q4=248 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits -region wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.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.SRN1xUZdTQ (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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits' -> 'wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
WCS_IMAGE_NAME=wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
WCS-calibrated image found: wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
Checking if the catalog wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat corresponding to the image wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits alredy exist and is non-empty...
Catalog wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat corresponding to the image wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
WCS catalog name: wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=384, passed=5181
Got 5181 stars (including 4792 good ones) from the SExtractor catalog wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat
util/solve_plate_with_UCAC5 got 5181 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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5151 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5149 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5149 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits N_match=979 sigma_overall_arcsec=0.481 sigma_q1_arcsec=0.431 sigma_q2_arcsec=0.511 sigma_q3_arcsec=0.417 sigma_q4_arcsec=0.567 n_q1=229 n_q2=263 n_q3=241 n_q4=246 worst_quadrant_to_overall_ratio=1.179
The image catalog is written to wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits -region wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.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.gdRe6CY55L (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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
WCS_IMAGE_NAME=wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
WCS-calibrated image found: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
Checking if the catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat corresponding to the image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat corresponding to the image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
WCS catalog name: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=399, passed=5738
Got 5738 stars (including 5339 good ones) from the SExtractor catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat
util/solve_plate_with_UCAC5 got 5738 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 5690 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 5689 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 5689 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits N_match=981 sigma_overall_arcsec=0.468 sigma_q1_arcsec=0.328 sigma_q2_arcsec=0.653 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.655 n_q1=243 n_q2=262 n_q3=249 n_q4=227 worst_quadrant_to_overall_ratio=1.400
The image catalog is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits -region wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.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.vaNulC9byr (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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
WCS_IMAGE_NAME=wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
WCS-calibrated image found: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
Checking if the catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat corresponding to the image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat corresponding to the image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
WCS catalog name: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=376, passed=5680
Got 5680 stars (including 5298 good ones) from the SExtractor catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat
util/solve_plate_with_UCAC5 got 5680 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 5634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 5636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 5636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits N_match=981 sigma_overall_arcsec=0.461 sigma_q1_arcsec=0.334 sigma_q2_arcsec=0.668 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.649 n_q1=241 n_q2=260 n_q3=252 n_q4=228 worst_quadrant_to_overall_ratio=1.448
The image catalog is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits -region wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits sigma_overall=0.379 worst_q_ratio=1.198
ref2=Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits sigma_overall=0.481 worst_q_ratio=1.179
new1=fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits sigma_overall=0.468 worst_q_ratio=1.400
new2=fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits sigma_overall=0.461 worst_q_ratio=1.448
reference average sigma_overall=0.43 worst_q_ratio=1.1885
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470_astrometric_residuals.png (980 matched stars from wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522_astrometric_residuals.png (979 matched stars from wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486_astrometric_residuals.png (981 matched stars from wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487_astrometric_residuals.png (981 matched stars from wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits'
Saving fully-calibrated image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits'
Preparing the HTML report for the field Vir-11-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:50:39.86 -09:37:20.3: 12.12 +/- 0.01 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:50:00.02 -10:05:53.3: 12.00 +/- 0.01 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:51:42.48 -11:15:03.4: 12.07 +/- 0.01 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:56:12.96 -11:03:49.7: 12.09 +/- 0.01 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:50:39.86 -09:37:20.3: 12.07 +/- 0.02 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:50:00.02 -10:05:53.3: 11.93 +/- 0.01 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:56:12.96 -11:03:49.7: 12.11 +/- 0.02 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:51:42.48 -11:15:03.4: 12.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry filter REJECTED candidate at 12:50:00.02 -10:05:53.3: ref_mag=11.97 +/- 0.01 new_mean_mag=11.9388 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 12:56:12.96 -11:03:49.7: ref_mag=12.10 +/- 0.01 new_mean_mag=12.0437 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter REJECTED candidate at 12:50:39.86 -09:37:20.3: ref_mag=12.10 +/- 0.01 new_mean_mag=12.0744 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 12:51:42.48 -11:15:03.4: ref_mag=12.09 +/- 0.01 new_mean_mag=12.0732 delta=0.01 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21188_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 21188_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21192_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 21192_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
**** FOUND 12:53:56.62 -10:47:06.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21194_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 21194_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
**** FOUND 12:39:34.19 -10:09:33.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21198_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 21198_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21200_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 21200_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21201_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 21201_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Vir-11-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/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
SExtractor catalog cache: saved Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat to cache
SExtractor catalog cache: saved Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
Creating symlink local_wcs_cache/wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.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_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits exists and is non-empty
wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits exists and is non-empty
wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits exists and is non-empty
wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits (1st reference image)
verification OK: wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
Image size: 941.6'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:51:17.659 -09:58:37.31 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits (1st new image)
verification OK: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
Image size: 936.8'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:51:26.385 -09:59:49.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:51:17.659 -09:58:37.31
Second-epoch image center 12:51:26.385 -09:59:49.21
Angular distance between the image centers 0.0410 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits (2nd new image)
verification OK: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
Image size: 936.8'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:51:26.014 -09:59:35.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:51:17.659 -09:58:37.31
Second-epoch image center 12:51:26.014 -09:59:35.01
Angular distance between the image centers 0.0378 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:51:26.385 -09:59:49.21
Second-epoch second image center 12:51:26.014 -09:59:35.01
Angular distance between the image centers 0.00423 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/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits &> /tmp/tmp.LTDkkBjwM1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits &> /tmp/tmp.dZHwLANKGY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits &> /tmp/tmp.8YBxpRwJdF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits &> /tmp/tmp.Ls8RAwN1LX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.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_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits and wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.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_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits and wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat
Found non-empty wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits and wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat
The reference image (wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits) and catalog (wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat) found
'wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat' -> 'wcsmag.cat'
Read 36963 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 184.7062 to 200.9373 deg, Dec -15.2672 to -4.6582 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 184.7062 to 200.9373 deg, Dec -15.2672 to -4.6582 deg
Loaded 4180 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): 3305 out of 3626 total matches.
Matched with Tycho-2 3626 out of 36963 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.748500
a=0.000000 b=1.000000 c=22.748500
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36963 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 184.7062 to 200.9373 deg, Dec -15.2672 to -4.6582 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 184.7062 to 200.9373 deg, Dec -15.2672 to -4.6582 deg
Loaded 4180 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): 3305 out of 3626 total matches.
Matched with Tycho-2 3626 out of 36963 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits:
Forced-photometry filter: calibrated wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits -> calib.txt_param_ref_wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits (aperture=4.5)
Read 31865 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 184.8992 to 201.0664 deg, Dec -15.3183 to -4.6060 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 184.8992 to 201.0664 deg, Dec -15.3183 to -4.6060 deg
Loaded 4196 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): 3339 out of 3563 total matches.
Matched with Tycho-2 3563 out of 31865 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits:
Forced-photometry filter: calibrated wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits -> calib.txt_param_ref_wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 28 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
2.1 pix Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
2.5 pix fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
2.5 pix fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
1.9 pix wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
2.1 pix wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
Limiting magnitude estimates:
15.3 mag. Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
15.0 mag. Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
15.0 mag. fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
15.0 mag. fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.LTDkkBjwM1 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits' -> 'wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
WCS_IMAGE_NAME=wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
WCS-calibrated image found: wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
Checking if the catalog wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat corresponding to the image wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits alredy exist and is non-empty...
Catalog wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat corresponding to the image wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits
WCS catalog name: wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1503, passed=36949
Got 36949 stars (including 35371 good ones) from the SExtractor catalog wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat
util/solve_plate_with_UCAC5 got 36949 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 36634 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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 36633 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 36633 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits N_match=981 sigma_overall_arcsec=0.375 sigma_q1_arcsec=0.445 sigma_q2_arcsec=0.343 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.346 n_q1=217 n_q2=270 n_q3=251 n_q4=243 worst_quadrant_to_overall_ratio=1.187
The image catalog is written to wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits -region wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.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.dZHwLANKGY (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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits' -> 'wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
WCS_IMAGE_NAME=wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
WCS-calibrated image found: wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
Checking if the catalog wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat corresponding to the image wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits alredy exist and is non-empty...
Catalog wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat corresponding to the image wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits
WCS catalog name: wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1223, passed=31851
Got 31851 stars (including 30581 good ones) from the SExtractor catalog wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat
util/solve_plate_with_UCAC5 got 31851 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 373 to 428 (Dec -15.3 to -4.6)
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(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 31550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 373 to 428 (Dec -15.3 to -4.6)
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(), 31551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 31551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits N_match=976 sigma_overall_arcsec=0.473 sigma_q1_arcsec=0.441 sigma_q2_arcsec=0.467 sigma_q3_arcsec=0.403 sigma_q4_arcsec=0.564 n_q1=215 n_q2=273 n_q3=236 n_q4=252 worst_quadrant_to_overall_ratio=1.191
The image catalog is written to wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits -region wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.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.8YBxpRwJdF (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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
WCS_IMAGE_NAME=wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
WCS-calibrated image found: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
Checking if the catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat corresponding to the image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat corresponding to the image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
WCS catalog name: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1817, passed=28637
Got 28637 stars (including 26785 good ones) from the SExtractor catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat
util/solve_plate_with_UCAC5 got 28637 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 28433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 28431 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 28430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits N_match=981 sigma_overall_arcsec=0.461 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.652 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.613 n_q1=241 n_q2=255 n_q3=268 n_q4=217 worst_quadrant_to_overall_ratio=1.414
The image catalog is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits -region wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.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.Ls8RAwN1LX (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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
WCS_IMAGE_NAME=wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
WCS-calibrated image found: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
Checking if the catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat corresponding to the image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat corresponding to the image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
WCS catalog name: wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1848, passed=28641
Got 28641 stars (including 26757 good ones) from the SExtractor catalog wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat
util/solve_plate_with_UCAC5 got 28641 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 28395 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 28397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 28397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits N_match=981 sigma_overall_arcsec=0.440 sigma_q1_arcsec=0.349 sigma_q2_arcsec=0.652 sigma_q3_arcsec=0.335 sigma_q4_arcsec=0.675 n_q1=247 n_q2=252 n_q3=269 n_q4=213 worst_quadrant_to_overall_ratio=1.533
The image catalog is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits -region wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-06_20.00sec_4.90C_LIGHT_1486.fits
Saving fully-calibrated image wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.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_2026-05-17_CI_Vir-11-Q2b1x1_233740_TTUQ2b1x1_2219744_r6mucJGI/wcs_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487.fits
Preparing the HTML report for the field Vir-11-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:50:48.91 -11:23:37.9: 13.51 +/- 0.04 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:07:13.85 -06:10:04.5: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:49:20.32 -08:21:34.5: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:06:55.07 -08:02:21.1: 14.17 +/- 0.08 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:08:44.12 -14:04:36.3: 14.87 +/- 0.17 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:59:33.85 -08:46:33.0: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:02:02.91 -10:24:46.7: 15.06 +/- 0.18 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:00:48.72 -12:00:24.4: 14.77 +/- 0.14 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:50:48.91 -11:23:37.9: 13.37 +/- 0.04 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:08:44.12 -14:04:36.3: 15.12 +/- 0.28 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:59:33.85 -08:46:33.0: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:07:13.85 -06:10:04.5: 15.58 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:49:20.32 -08:21:34.5: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:06:55.07 -08:02:21.1: 14.15 +/- 0.10 detection
Forced photometry filter REJECTED candidate at 12:50:48.91 -11:23:37.9: ref_mag=13.45 +/- 0.03 new_mean_mag=13.4961 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 14.93 +/- 0.14
Forced photometry filter REJECTED candidate at 13:08:44.12 -14:04:36.3: ref_mag=14.93 +/- 0.14 new_mean_mag=14.5099 delta=0.42 (need > 0.90)
Forced photometry reference-image weighted average: 14.16 +/- 0.06
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:02:31.34 -05:44:34.7: 15.10 +/- 0.17 detection
Forced photometry filter REJECTED candidate at 13:06:55.07 -08:02:21.1: ref_mag=14.16 +/- 0.06 new_mean_mag=14.2841 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:02:02.91 -10:24:46.7: 14.75 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.12
Forced photometry filter REJECTED candidate at 13:02:02.91 -10:24:46.7: ref_mag=14.90 +/- 0.12 new_mean_mag=14.4754 delta=0.42 (need > 0.90)
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:00:48.72 -12:00:24.4: 14.69 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.10
Forced photometry filter REJECTED candidate at 13:00:48.72 -12:00:24.4: ref_mag=14.74 +/- 0.10 new_mean_mag=14.5142 delta=0.22 (need > 0.90)
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:02:31.34 -05:44:34.7: 14.84 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.12
Forced photometry filter REJECTED candidate at 13:02:31.34 -05:44:34.7: ref_mag=14.96 +/- 0.12 new_mean_mag=14.6345 delta=0.33 (need > 0.90)
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:02:25.85 -12:47:41.2: 15.35 +/- 0.23 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:08:32.95 -10:27:37.3: 15.15 +/- 0.21 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:08:47.91 -05:46:00.3: 15.03 +/- 0.17 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:56:10.29 -11:03:01.9: 15.15 +/- 0.18 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:09:05.40 -13:39:56.8: 14.86 +/- 0.16 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:05:02.23 -13:14:10.8: 15.06 +/- 0.19 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:02:25.85 -12:47:41.2: 14.93 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.15
Forced photometry filter REJECTED candidate at 13:02:25.85 -12:47:41.2: ref_mag=15.11 +/- 0.15 new_mean_mag=14.7586 delta=0.35 (need > 0.90)
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:08:32.95 -10:27:37.3: 14.79 +/- 0.18 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:08:47.91 -05:46:00.3: 15.11 +/- 0.24 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:56:10.29 -11:03:01.9: 14.92 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.14
Forced photometry reference-image weighted average: 15.06 +/- 0.14
Forced photometry filter REJECTED candidate at 13:08:32.95 -10:27:37.3: ref_mag=14.95 +/- 0.14 new_mean_mag=14.7688 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 15.04 +/- 0.13
Forced photometry filter REJECTED candidate at 13:08:47.91 -05:46:00.3: ref_mag=15.06 +/- 0.14 new_mean_mag=14.6326 delta=0.42 (need > 0.90)
Forced photometry filter REJECTED candidate at 12:56:10.29 -11:03:01.9: ref_mag=15.04 +/- 0.13 new_mean_mag=14.8060 delta=0.23 (need > 0.90)
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:07:07.35 -12:22:01.3: 14.95 +/- 0.17 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:09:05.40 -13:39:56.8: 14.86 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.13
Forced photometry filter REJECTED candidate at 13:09:05.40 -13:39:56.8: ref_mag=14.86 +/- 0.13 new_mean_mag=14.6542 delta=0.20 (need > 0.90)
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:05:02.23 -13:14:10.8: 14.73 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.13
Forced photometry filter REJECTED candidate at 13:05:02.23 -13:14:10.8: ref_mag=14.88 +/- 0.13 new_mean_mag=14.8542 delta=0.03 (need > 0.90)
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:07:07.35 -12:22:01.3: 14.83 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.12
Forced photometry filter REJECTED candidate at 13:07:07.35 -12:22:01.3: ref_mag=14.89 +/- 0.12 new_mean_mag=14.8242 delta=0.07 (need > 0.90)
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:52:08.10 -06:37:21.8: 15.90 +/- 0.35 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:58:53.27 -07:05:51.4: 15.14 +/- 0.18 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 13:05:37.42 -13:31:14.3: 14.86 +/- 0.16 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-02-11_03-58-54_20.00sec_-14.90C_LIGHT_0470.fits at 12:59:43.11 -08:05:56.6: 15.14 +/- 0.18 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:52:08.10 -06:37:21.8: 15.40 +/- 0.27 detection
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:58:53.27 -07:05:51.4: 15.05 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.59 +/- 0.21
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 13:05:37.42 -13:31:14.3: 14.64 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 12:52:08.10 -06:37:21.8: ref_mag=15.59 +/- 0.21 new_mean_mag=14.7474 delta=0.84 (need > 0.90)
Forced photometry reference-image weighted average: 15.10 +/- 0.14
Forced photometry filter REJECTED candidate at 12:58:53.27 -07:05:51.4: ref_mag=15.10 +/- 0.14 new_mean_mag=14.9210 delta=0.18 (need > 0.90)
Forced photometry on wcs_Vir-11-Q2b1x1_2026-04-19_00-58-29_20.00sec_-4.90C_LIGHT_0522.fits at 12:59:43.11 -08:05:56.6: 15.23 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.11
Forced photometry filter REJECTED candidate at 13:05:37.42 -13:31:14.3: ref_mag=14.75 +/- 0.11 new_mean_mag=14.8908 delta=-0.14 (need > 0.90)
Forced photometry reference-image weighted average: 15.17 +/- 0.14
Forced photometry filter REJECTED candidate at 12:59:43.11 -08:05:56.6: ref_mag=15.17 +/- 0.14 new_mean_mag=14.8374 delta=0.34 (need > 0.90)
Adding exclusion_list_local.txt__out56845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56856.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
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Considering the candidate 56808_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 56808_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 56818_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 56818_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 56821_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 56821_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 56845_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
Preparing report for the candidate 56845_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
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Considering the candidate 56846_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
Preparing report for the candidate 56846_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
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Considering the candidate 56848_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 56848_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 56856_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
Preparing report for the candidate 56856_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
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Considering the candidate 56868_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 56868_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
**** FOUND 12:52:09.88 -06:04:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56937_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 56937_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57124_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57124_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57230_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57230_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
**** FOUND 13:08:20.86 -13:10:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57273_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57273_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57303_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57303_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 57315_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57315_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57375_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57375_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
**** FOUND 12:57:59.98 -13:12:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57469_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57469_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57552_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57552_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
**** FOUND 13:02:02.33 -07:56:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57586_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57586_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57606_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57606_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57627_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57627_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57628_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57628_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57657_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57657_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57660_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57660_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57674_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57674_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57696_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57696_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57715_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57715_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57773_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57773_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks
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Considering the candidate 57781_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487
The candidate 57781_fd_Vir-11-Q2b1x1_2026-05-17_23-33-44_20.00sec_4.90C_LIGHT_1487 did not pass the final checks