This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 09.2929 2461200.7929 12.48 14:05:23.22 -10:19:09.8
331.00638 48.47994 galactic Vir Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.79 Eurynome -0 -0 0 12.5 0 -0
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 14:05:23.22 -10:19:09.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 14:05:23.22 -10:19:09.8: 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 06 09.2929* 14 05 23.22 -10 19 09.8 12.5 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,2461200.7929,12.48,0.05,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 20260609.2929 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.2929 2461200.7929 13.36 13:52:48.68 -12:18:40.6
325.58653 47.84258 galactic Vir Second-epoch detections are separated by 0.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.599 Luisa 0 1 1 13.4 0 -0
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:52:48.68 -12:18:40.6: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:52:48.68 -12:18:40.6: 15.79 +/- 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 06 09.2929* 13 52 48.68 -12 18 40.6 13.4 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,2461200.7929,13.36,0.05,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 20260609.2929 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.2929 2461200.7929 13.48 13:31:44.80 -13:00:22.9
317.89889 48.69048 galactic Vir Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.142 Polana -0 -1 1 13.8 -0 -0
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:31:44.80 -13:00:22.9: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:31:44.80 -13:00:22.9: 15.80 +/- 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 06 09.2929* 13 31 44.80 -13 00 22.9 13.5 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,2461200.7929,13.48,0.05,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 20260609.2929 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.2929 2461200.7929 13.54 13:28:27.22 -11:27:03.9
317.24401 50.38920 galactic Vir Second-epoch detections are separated by 3.0" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.77 Frigga -1 -0 1 13.6 -0 -0
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:28:27.22 -11:27:03.9: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:28:27.22 -11:27:03.9: 15.83 +/- 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 06 09.2929* 13 28 27.22 -11 27 03.9 13.5 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,2461200.7929,13.54,0.05,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 20260609.2929 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.2929 2461200.7929 14.01 13:35:20.26 -07:07:15.2
321.74470 54.13957 galactic Vir Second-epoch detections are separated by 2.2" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.240 Vanadis -1 0 1 14.5 -0 0
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:35:20.26 -07:07:15.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:35:20.26 -07:07:15.2: 15.91 +/- 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 06 09.2929* 13 35 20.26 -07 07 15.2 14.0 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,2461200.7929,14.01,0.05,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 20260609.2929 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.2929 2461200.7929 14.17 13:57:44.24 -13:03:13.3
326.84372 46.71682 galactic Vir Second-epoch detections are separated by 1.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.342 Endymion 1 -1 2 14.7 -0 -0
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:57:44.24 -13:03:13.3: 15.44 +/- 0.29 detection
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:57:44.24 -13:03:13.3: 15.71 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.44 +/- 0.29
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 06 09.2929* 13 57 44.24 -13 03 13.3 14.2 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,2461200.7929,14.17,0.05,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 20260609.2929 14.17CV 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: 2461172.73798667 12.05.2026 05:42:32.048 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
First image: 2461172.73798667 12.05.2026 05:42:32.048 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
Last image: 2461200.79322588 09.06.2026 07:02:04.716 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.69
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4546
Objects passed selection criteria: 4541
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 4182.5
Average stars matched: 4113 (98.3383 %)
Memory usage VmPeak: 111180 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 9 02:25:53 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: 2461172.73798667 12.05.2026 05:42:32.048 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
First image: 2461172.73798667 12.05.2026 05:42:32.048 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
Last image: 2461200.79322588 09.06.2026 07:02:04.716 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 24 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): 28279
Objects passed selection criteria: 28233
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 25271.8
Average stars matched: 24616.5 (97.4072 %)
Memory usage VmPeak: 133408 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 9 02:28:26 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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.cat to cache
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.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: 2461200.79257949
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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits exists and is non-empty
Saving wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits to local_wcs_cache/
'wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits' -> 'local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits'
wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits exists and is non-empty
Saving wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits to local_wcs_cache/
'wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits' -> 'local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits'
wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits exists and is non-empty
Saving wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits to local_wcs_cache/
'wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits' -> 'local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits'
wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits exists and is non-empty
Saving wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits to local_wcs_cache/
'wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits' -> 'local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits (1st reference image)
verification OK: wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:52.315 -09:59:49.65 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits (1st new image)
verification OK: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:52.292 -10:00:22.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:42:52.315 -09:59:49.65
Second-epoch image center 13:42:52.292 -10:00:22.24
Angular distance between the image centers 0.0091 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits (2nd new image)
verification OK: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:55.167 -10:00:48.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:42:52.315 -09:59:49.65
Second-epoch image center 13:42:55.167 -10:00:48.14
Angular distance between the image centers 0.0200 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 13:42:52.292 -10:00:22.24
Second-epoch second image center 13:42:55.167 -10:00:48.14
Angular distance between the image centers 0.01382 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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits &> /tmp/tmp.mETbRjfUXq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits &> /tmp/tmp.nAXKYGzh4l
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits &> /tmp/tmp.YNGuo7nsSE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits &> /tmp/tmp.bNOD8Jh5ZG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat
Found non-empty wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat
The reference image (wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits) and catalog (wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat) found
'wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat' -> 'wcsmag.cat'
Read 6188 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6939 to 213.7936 deg, Dec -15.2572 to -4.7129 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 197.6939 to 213.7936 deg, Dec -15.2572 to -4.7129 deg
Loaded 4351 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): 3563 out of 3677 total matches.
Matched with Tycho-2 3677 out of 6188 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.740200
a=0.000000 b=1.000000 c=22.740200
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.05
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.05
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6188 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6939 to 213.7936 deg, Dec -15.2572 to -4.7129 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 197.6939 to 213.7936 deg, Dec -15.2572 to -4.7129 deg
Loaded 4351 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): 3563 out of 3677 total matches.
Matched with Tycho-2 3677 out of 6188 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits:
Forced-photometry filter: calibrated wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits -> calib.txt_param_ref_wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits (aperture=6.1)
Read 6192 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6939 to 213.8142 deg, Dec -15.2663 to -4.7279 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 197.6939 to 213.8142 deg, Dec -15.2663 to -4.7279 deg
Loaded 4358 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): 3560 out of 3677 total matches.
Matched with Tycho-2 3677 out of 6192 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits:
Forced-photometry filter: calibrated wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits -> calib.txt_param_ref_wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
2.2 pix Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
2.5 pix fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
2.5 pix fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
2.2 pix wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
2.2 pix wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
Limiting magnitude estimates:
15.0 mag. Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
15.0 mag. Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
14.4 mag. fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
14.4 mag. fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mETbRjfUXq (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_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits' -> 'wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=399, passed=6188
Got 6188 stars (including 5785 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat
util/solve_plate_with_UCAC5 got 6188 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 6109 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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 6111 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 6111 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits N_match=975 sigma_overall_arcsec=0.496 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.585 sigma_q3_arcsec=0.441 sigma_q4_arcsec=0.549 n_q1=236 n_q2=237 n_q3=240 n_q4=262 worst_quadrant_to_overall_ratio=1.181
The image catalog is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits -region wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nAXKYGzh4l (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_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.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-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits' -> 'wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat corresponding to the image wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat corresponding to the image wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=409, passed=6192
Got 6192 stars (including 5778 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat
util/solve_plate_with_UCAC5 got 6192 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 6116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 6117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 6117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits N_match=975 sigma_overall_arcsec=0.496 sigma_q1_arcsec=0.391 sigma_q2_arcsec=0.621 sigma_q3_arcsec=0.410 sigma_q4_arcsec=0.532 n_q1=245 n_q2=234 n_q3=230 n_q4=266 worst_quadrant_to_overall_ratio=1.253
The image catalog is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits -region wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.YNGuo7nsSE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=275, passed=4329
Got 4329 stars (including 4053 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat
util/solve_plate_with_UCAC5 got 4329 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 -4.7)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 4261 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 -4.7)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 4259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 4259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits N_match=974 sigma_overall_arcsec=0.554 sigma_q1_arcsec=0.459 sigma_q2_arcsec=0.665 sigma_q3_arcsec=0.522 sigma_q4_arcsec=0.604 n_q1=272 n_q2=209 n_q3=261 n_q4=232 worst_quadrant_to_overall_ratio=1.200
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits -region wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bNOD8Jh5ZG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=287, passed=4315
Got 4315 stars (including 4028 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat
util/solve_plate_with_UCAC5 got 4315 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 -4.7)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 4229 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 -4.7)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 4231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 4231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits N_match=975 sigma_overall_arcsec=0.559 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.722 sigma_q3_arcsec=0.483 sigma_q4_arcsec=0.691 n_q1=270 n_q2=208 n_q3=258 n_q4=239 worst_quadrant_to_overall_ratio=1.291
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits -region wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits sigma_overall=0.496 worst_q_ratio=1.181
ref2=Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits sigma_overall=0.496 worst_q_ratio=1.253
new1=fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits sigma_overall=0.554 worst_q_ratio=1.200
new2=fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits sigma_overall=0.559 worst_q_ratio=1.291
reference average sigma_overall=0.496 worst_q_ratio=1.217
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166_astrometric_residuals.png (975 matched stars from wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167_astrometric_residuals.png (975 matched stars from wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104_astrometric_residuals.png (974 matched stars from wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105_astrometric_residuals.png (975 matched stars from wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits'
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits'
Preparing the HTML report for the field Vir-12-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20267_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
The candidate 20267_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105 did not pass the final checks
**** FOUND 13:55:24.41 -09:13:00.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Vir-12-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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.cat to cache
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
Creating symlink local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits exists and is non-empty
wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits exists and is non-empty
wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits exists and is non-empty
wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits (1st reference image)
verification OK: wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:52.315 -09:59:49.65 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits (1st new image)
verification OK: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:52.292 -10:00:22.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:42:52.315 -09:59:49.65
Second-epoch image center 13:42:52.292 -10:00:22.24
Angular distance between the image centers 0.0091 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits (2nd new image)
verification OK: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:55.167 -10:00:48.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:42:52.315 -09:59:49.65
Second-epoch image center 13:42:55.167 -10:00:48.14
Angular distance between the image centers 0.0200 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 13:42:52.292 -10:00:22.24
Second-epoch second image center 13:42:55.167 -10:00:48.14
Angular distance between the image centers 0.01382 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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits &> /tmp/tmp.j0MAQV3ENT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits &> /tmp/tmp.2Y3OnJbPy7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits &> /tmp/tmp.H5liXNwOiB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits &> /tmp/tmp.ehnXFbLSVI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat
Found non-empty wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat
The reference image (wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits) and catalog (wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat) found
'wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat' -> 'wcsmag.cat'
Read 36085 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6538 to 213.8134 deg, Dec -15.2617 to -4.6907 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 197.6538 to 213.8134 deg, Dec -15.2617 to -4.6907 deg
Loaded 4373 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): 3495 out of 3774 total matches.
Matched with Tycho-2 3774 out of 36085 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.605600
a=0.000000 b=1.000000 c=22.605600
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36085 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6538 to 213.8134 deg, Dec -15.2617 to -4.6907 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 197.6538 to 213.8134 deg, Dec -15.2617 to -4.6907 deg
Loaded 4373 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): 3495 out of 3774 total matches.
Matched with Tycho-2 3774 out of 36085 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits:
Forced-photometry filter: calibrated wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits -> calib.txt_param_ref_wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits (aperture=4.7)
Read 36122 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6619 to 213.8224 deg, Dec -15.2704 to -4.6959 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 197.6619 to 213.8224 deg, Dec -15.2704 to -4.6959 deg
Loaded 4378 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): 3491 out of 3773 total matches.
Matched with Tycho-2 3773 out of 36122 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits:
Forced-photometry filter: calibrated wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits -> calib.txt_param_ref_wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
2.1 pix Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
2.5 pix fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
2.5 pix fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
2.1 pix wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
2.1 pix wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
Limiting magnitude estimates:
15.2 mag. Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
15.2 mag. Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
14.6 mag. fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
14.6 mag. fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (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.j0MAQV3ENT (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_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits' -> 'wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1598, passed=36071
Got 36071 stars (including 34420 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat
util/solve_plate_with_UCAC5 got 36071 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 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(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 35611 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
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(), 35612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 35612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits N_match=976 sigma_overall_arcsec=0.465 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.539 sigma_q3_arcsec=0.411 sigma_q4_arcsec=0.526 n_q1=250 n_q2=240 n_q3=234 n_q4=252 worst_quadrant_to_overall_ratio=1.158
The image catalog is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits -region wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2Y3OnJbPy7 (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_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.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-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits' -> 'wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat corresponding to the image wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat corresponding to the image wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1643, passed=36115
Got 36115 stars (including 34429 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat
util/solve_plate_with_UCAC5 got 36115 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 35632 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 35631 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 35629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits N_match=975 sigma_overall_arcsec=0.491 sigma_q1_arcsec=0.415 sigma_q2_arcsec=0.567 sigma_q3_arcsec=0.402 sigma_q4_arcsec=0.512 n_q1=256 n_q2=241 n_q3=223 n_q4=255 worst_quadrant_to_overall_ratio=1.154
The image catalog is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits -region wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.H5liXNwOiB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1269, passed=23220
Got 23220 stars (including 21936 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat
util/solve_plate_with_UCAC5 got 23220 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 -4.7)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 22817 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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 22814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 22814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits N_match=973 sigma_overall_arcsec=0.534 sigma_q1_arcsec=0.459 sigma_q2_arcsec=0.617 sigma_q3_arcsec=0.505 sigma_q4_arcsec=0.584 n_q1=289 n_q2=196 n_q3=264 n_q4=224 worst_quadrant_to_overall_ratio=1.156
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits -region wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ehnXFbLSVI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1257, passed=23220
Got 23220 stars (including 21938 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat
util/solve_plate_with_UCAC5 got 23220 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 -4.7)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 22776 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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 22776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 22776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits N_match=974 sigma_overall_arcsec=0.555 sigma_q1_arcsec=0.434 sigma_q2_arcsec=0.720 sigma_q3_arcsec=0.495 sigma_q4_arcsec=0.646 n_q1=284 n_q2=196 n_q3=266 n_q4=228 worst_quadrant_to_overall_ratio=1.296
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits -region wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-01-08_20.00sec_4.90C_LIGHT_0104.fits
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Vir-12-Q2b1x1_022210_TTUQ2b1x1_245890_WzCpeulJ/wcs_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105.fits
Preparing the HTML report for the field Vir-12-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:31:44.80 -13:00:22.9: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:38:18.57 -12:25:30.9: 14.05 +/- 0.07 detection
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:46:45.36 -12:01:53.1: 13.67 +/- 0.05 detection
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 14:05:23.22 -10:19:09.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:52:48.68 -12:18:40.6: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:28:27.22 -11:27:03.9: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:35:20.26 -07:07:15.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 13:57:44.24 -13:03:13.3: 15.44 +/- 0.29 detection
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 14:03:40.37 -10:16:22.8: 14.54 +/- 0.13 detection
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-42-32_20.00sec_-4.90C_LIGHT_0166.fits at 14:03:18.73 -11:24:36.8: 14.91 +/- 0.18 detection
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:31:44.80 -13:00:22.9: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:38:18.57 -12:25:30.9: 13.84 +/- 0.06 detection
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 14:05:23.22 -10:19:09.8: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:46:45.36 -12:01:53.1: 13.77 +/- 0.05 detection
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:28:27.22 -11:27:03.9: 15.83 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Forced photometry filter REJECTED candidate at 13:38:18.57 -12:25:30.9: ref_mag=13.93 +/- 0.05 new_mean_mag=13.7359 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 13:46:45.36 -12:01:53.1: ref_mag=13.71 +/- 0.04 new_mean_mag=13.5213 delta=0.19 (need > 0.90)
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:52:48.68 -12:18:40.6: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:35:20.26 -07:07:15.2: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 13:57:44.24 -13:03:13.3: 15.71 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.44 +/- 0.29
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 14:03:40.37 -10:16:22.8: 14.88 +/- 0.18 detection
Forced photometry filter KEPT candidate at 13:57:44.24 -13:03:13.3: ref_mag=15.44 +/- 0.29 new_mean_mag=14.1689 delta=1.27 (need > 0.90)
Forced photometry on wcs_Vir-12-Q2b1x1_2026-05-12_00-43-21_20.00sec_-5.00C_LIGHT_0167.fits at 14:03:18.73 -11:24:36.8: 14.99 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.10
Forced photometry filter REJECTED candidate at 14:03:40.37 -10:16:22.8: ref_mag=14.65 +/- 0.10 new_mean_mag=14.3621 delta=0.29 (need > 0.90)
Forced photometry reference-image weighted average: 14.95 +/- 0.13
Forced photometry filter REJECTED candidate at 14:03:18.73 -11:24:36.8: ref_mag=14.95 +/- 0.13 new_mean_mag=14.6225 delta=0.32 (need > 0.90)
Adding exclusion_list_local.txt__out52415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52484.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 46s
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: 4s
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Considering the candidate 52389_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
The candidate 52389_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105 did not pass the final checks
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Considering the candidate 52390_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
The candidate 52390_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105 did not pass the final checks
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Considering the candidate 52415_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
Preparing report for the candidate 52415_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
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Considering the candidate 52430_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
The candidate 52430_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105 did not pass the final checks
**** FOUND 14:01:10.11 -09:15:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52441_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
The candidate 52441_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105 did not pass the final checks
**** FOUND 14:05:34.64 -08:13:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52448_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
The candidate 52448_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105 did not pass the final checks
**** FOUND 14:08:11.61 -10:25:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52458_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
Preparing report for the candidate 52458_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
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Considering the candidate 52466_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
The candidate 52466_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105 did not pass the final checks
**** FOUND 13:44:18.83 -12:57:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52469_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
Preparing report for the candidate 52469_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
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Considering the candidate 52475_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
Preparing report for the candidate 52475_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
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Considering the candidate 52482_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
Preparing report for the candidate 52482_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
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Considering the candidate 52484_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
Preparing report for the candidate 52484_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
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Considering the candidate 52511_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
The candidate 52511_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105 did not pass the final checks
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Considering the candidate 52512_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105
The candidate 52512_fd_Vir-12-Q2b1x1_2026-06-09_02-02-04_20.00sec_5.00C_LIGHT_0105 did not pass the final checks