This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy
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 09 01.2505 2461284.7505 12.32 04:20:28.86 +45:50:16.1
156.41599 -3.00381 galactic Per Second-epoch detections are separated by 2.3" and 5.8 pix
The object was found in VSX 7" NSVS J0420294+455021
Type: L
# Max. Min./Amp. JD0 Period
11.242 R1 Y 0.946 R1 400.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:20:28.86 +45:50:16.1: 13.26 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:20:28.86 +45:50:16.1: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
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 09 01.2505* 04 20 28.86 +45 50 16.1 12.3 U Per 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
NSVS J0420294+455021,2461284.7505,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0420294+455021 20260901.2505 12.32CV 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 09 01.2505 2461284.7505 12.35 04:49:53.47 +49:03:28.6
157.40161 2.83346 galactic Per Second-epoch detections are separated by 2.3" and 5.0 pix
The object was found in VSX 1" ASASSN-V J044953.55+490329.4
Type: SR
# Max. Min./Amp. JD0 Period
13.310 V 13.650 V 2458513.75110 51.965813300000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:49:53.47 +49:03:28.6: 13.26 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:49:53.47 +49:03:28.6: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
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 09 01.2505* 04 49 53.47 +49 03 28.6 12.3 U Per 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
ASASSN-V J044953.55+490329.4,2461284.7505,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J044953.55+490329.4 20260901.2505 12.35CV 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 09 01.2505 2461284.7505 12.00 04:37:47.91 +42:27:40.1
161.00868 -3.07806 galactic Per Second-epoch detections are separated by 0.8" and 5.8 pix
The object was found in VSX 1" ASASSN-V J043747.78+422740.0
Type: L
# Max. Min./Amp. JD0 Period
12.890 V 13.320 V
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:37:47.91 +42:27:40.1: 12.90 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:37:47.91 +42:27:40.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
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 09 01.2505* 04 37 47.91 +42 27 40.1 12.0 U Per 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
ASASSN-V J043747.78+422740.0,2461284.7505,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J043747.78+422740.0 20260901.2505 12.00CV 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 09 01.2505 2461284.7505 11.63 04:38:32.01 +42:28:05.1
161.09409 -2.97248 galactic Per Second-epoch detections are separated by 1.0" and 5.6 pix
The object was found in VSX 1" ASASSN-V J043831.90+422804.8
Type: SR
# Max. Min./Amp. JD0 Period
13.830 g Y 0.390 g 2458561.69700 179.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:38:32.01 +42:28:05.1: 12.63 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:38:32.01 +42:28:05.1: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
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 09 01.2505* 04 38 32.01 +42 28 05.1 11.6 U Per 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
ASASSN-V J043831.90+422804.8,2461284.7505,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J043831.90+422804.8 20260901.2505 11.63CV 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 09 01.2505 2461284.7505 11.15 04:40:30.28 +43:11:52.4
160.78847 -2.21749 galactic Per Second-epoch detections are separated by 0.9" and 5.5 pix
The object was found in VSX 1" V0748 Per
Type: LB
# Max. Min./Amp. JD0 Period
10.200 w 10.600 w 282.000000000000 C(N)
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:40:30.28 +43:11:52.4: 12.11 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:40:30.28 +43:11:52.4: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
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 09 01.2505* 04 40 30.28 +43 11 52.4 11.2 U Per 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
V0748 Per,2461284.7505,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
V0748 Per 20260901.2505 11.15CV 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 09 01.2505 2461284.7505 10.49 04:53:15.55 +41:48:57.0
163.36465 -1.32097 galactic Aur Second-epoch detections are separated by 0.6" and 5.5 pix
The object was found in VSX 0" EY Aur
Type: M
# Max. Min./Amp. JD0 Period
11.600 V 13.700 V 2428116.00000 270.000000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:53:15.55 +41:48:57.0: 11.45 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:53:15.55 +41:48:57.0: 11.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.00
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!
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
EY Aur,2461284.7505,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
EY Aur 20260901.2505 10.49CV 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: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
First image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Last image: 2461284.75076406 01.09.2026 06:00:56.015 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
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: 6 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 22127
Objects passed selection criteria: 21954
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 13703
Average stars matched: 13266 (96.8109 %)
Memory usage VmPeak: 247004 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 1 01:03:06 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: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
First image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Last image: 2461284.75076406 01.09.2026 06:00:56.015 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 60
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.37
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: 29 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 177261
Objects passed selection criteria: 176680
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 113306
Average stars matched: 108564 (95.8155 %)
Memory usage VmPeak: 640652 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 1 01:05:05 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/TTUQ1b1x1/TTUQ1_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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
SExtractor catalog cache: saved Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.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/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.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: 2461284.75019653
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_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits exists and is non-empty
wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (1st reference image)
verification OK: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:00.727 +45:59:45.06 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits (1st new image)
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
Image size: 944.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:47:56.593 +46:00:17.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:47:56.593 +46:00:17.20
Angular distance between the image centers 0.0149 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits (2nd new image)
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
Image size: 944.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:47:59.615 +46:00:10.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:47:59.615 +46:00:10.36
Angular distance between the image centers 0.0077 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 04:47:56.593 +46:00:17.20
Second-epoch second image center 04:47:59.615 +46:00:10.36
Angular distance between the image centers 0.00895 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.HaGKNZeCl5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.4mXYMYeBSO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits &> /tmp/tmp.Wdl5jShpZO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits &> /tmp/tmp.4BvitrMdVP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.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_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.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_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Found non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
The reference image (wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits) and catalog (wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat) found
'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat' -> 'wcsmag.cat'
Read 23847 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9496 to 84.6399 deg, Dec +39.9317 to +51.3292 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 59.9496 to 84.6399 deg, Dec 39.9317 to 51.3292 deg
Loaded 12139 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): 8124 out of 9276 total matches.
Matched with Tycho-2 9276 out of 23847 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.951350
a=0.000000 b=1.000000 c=22.951350
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23847 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9496 to 84.6399 deg, Dec +39.9317 to +51.3292 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 59.9496 to 84.6399 deg, Dec 39.9317 to 51.3292 deg
Loaded 12139 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): 8124 out of 9276 total matches.
Matched with Tycho-2 9276 out of 23847 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Forced-photometry filter: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -> calib.txt_param_ref_wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (aperture=6.1)
Read 23965 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9494 to 84.6297 deg, Dec +39.9321 to +51.3293 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 59.9494 to 84.6297 deg, Dec 39.9321 to 51.3293 deg
Loaded 12131 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): 8135 out of 9280 total matches.
Matched with Tycho-2 9280 out of 23965 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Forced-photometry filter: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -> calib.txt_param_ref_wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
2.1 pix Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
2.8 pix fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
2.8 pix fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
Limiting magnitude estimates:
15.2 mag. Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
15.2 mag. Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
12.8 mag. fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
12.8 mag. fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.5 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.HaGKNZeCl5 (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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2564, bad_region=0, passed=23847
Got 23847 stars (including 21254 good ones) from the SExtractor catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
util/solve_plate_with_UCAC5 got 23847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 4871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 23847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 23847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 23847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4872 stars left (next iteration limit 5358)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits N_match=4872 sigma_overall_arcsec=0.443 sigma_q1_arcsec=0.581 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.440 sigma_q4_arcsec=0.341 n_q1=1102 n_q2=1035 n_q3=1609 n_q4=1126 worst_quadrant_to_overall_ratio=1.312
The image catalog is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.4mXYMYeBSO (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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2577, bad_region=0, passed=23965
Got 23965 stars (including 21358 good ones) from the SExtractor catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
util/solve_plate_with_UCAC5 got 23965 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 23965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 23965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 23965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4869 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits N_match=4869 sigma_overall_arcsec=0.448 sigma_q1_arcsec=0.587 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.343 n_q1=1104 n_q2=1036 n_q3=1603 n_q4=1126 worst_quadrant_to_overall_ratio=1.308
The image catalog is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Wdl5jShpZO (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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
WCS-calibrated image found: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
Checking if the catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
WCS catalog name: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=239, bad_region=0, passed=3703
Got 3703 stars (including 3462 good ones) from the SExtractor catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat
util/solve_plate_with_UCAC5 got 3703 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.4)
Done reading UCAC5 zone files...
Matched 3393 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3349 matched stars entering correct_measured_positions(), 3344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3349 matched stars entering correct_measured_positions(), 3698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.4)
Done reading UCAC5 zone files...
Matched 3394 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3350 matched stars entering correct_measured_positions(), 3698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 3349 matched stars entering correct_measured_positions(), 3698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 3349 stars left (next iteration limit 3683)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3349 robust_rms=8.475 arcsec worst_quadrant_rms=13.381 arcsec
SIP_REFIT: SIP order 3 trial: matched=3349 robust_rms=0.772 arcsec worst_quadrant_rms=1.379 arcsec
SIP_REFIT: SIP order 5 trial: matched=3349 robust_rms=0.630 arcsec worst_quadrant_rms=0.984 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3349 robust_rms_before=1.407 arcsec robust_rms_before_corrected=0.588 arcsec robust_rms_after=0.630 arcsec worst_quadrant_rms_before=0.886 worst_quadrant_rms_after=0.984
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.886 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits N_match=3349 sigma_overall_arcsec=0.565 sigma_q1_arcsec=0.552 sigma_q2_arcsec=0.912 sigma_q3_arcsec=0.373 sigma_q4_arcsec=0.703 n_q1=960 n_q2=665 n_q3=976 n_q4=748 worst_quadrant_to_overall_ratio=1.613
The image catalog is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits -region wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.4BvitrMdVP (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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
WCS-calibrated image found: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
Checking if the catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
WCS catalog name: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=253, bad_region=0, passed=3704
Got 3704 stars (including 3450 good ones) from the SExtractor catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat
util/solve_plate_with_UCAC5 got 3704 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 3385 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3341 matched stars entering correct_measured_positions(), 3339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3340 matched stars entering correct_measured_positions(), 3700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 3386 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3340 matched stars entering correct_measured_positions(), 3700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 3340 matched stars entering correct_measured_positions(), 3700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 3340 stars left (next iteration limit 3674)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3340 robust_rms=8.609 arcsec worst_quadrant_rms=12.324 arcsec
SIP_REFIT: SIP order 3 trial: matched=3340 robust_rms=0.766 arcsec worst_quadrant_rms=1.191 arcsec
SIP_REFIT: SIP order 5 trial: matched=3340 robust_rms=0.612 arcsec worst_quadrant_rms=1.007 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3340 robust_rms_before=1.427 arcsec robust_rms_before_corrected=0.563 arcsec robust_rms_after=0.612 arcsec worst_quadrant_rms_before=0.894 worst_quadrant_rms_after=1.007
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.894 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits N_match=3340 sigma_overall_arcsec=0.568 sigma_q1_arcsec=0.536 sigma_q2_arcsec=0.894 sigma_q3_arcsec=0.416 sigma_q4_arcsec=0.630 n_q1=980 n_q2=692 n_q3=930 n_q4=738 worst_quadrant_to_overall_ratio=1.574
The image catalog is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits -region wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
Saving the final (post-refit) wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits to local_wcs_cache/
'wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'local_wcs_cache/wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
Saving the final (post-refit) wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits to local_wcs_cache/
'wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits'
Saving the final (post-refit) wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits to local_wcs_cache/
'wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits sigma_overall=0.443 worst_q_ratio=1.312
ref2=Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits sigma_overall=0.448 worst_q_ratio=1.308
new1=fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits sigma_overall=0.565 worst_q_ratio=1.613
new2=fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits sigma_overall=0.568 worst_q_ratio=1.574
reference average sigma_overall=0.4455 worst_q_ratio=1.31
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044_astrometric_residuals.png (4872 matched stars from wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045_astrometric_residuals.png (4869 matched stars from wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228_astrometric_residuals.png (3349 matched stars from wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229_astrometric_residuals.png (3340 matched stars from wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits'
Saving fully-calibrated image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits'
Preparing the HTML report for the field Per-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31731_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 31731_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:32:36.72 +45:40:13.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02488_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 02488_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:54:15.09 +49:53:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00847_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 00847_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:27:03.87 +50:07:25.3 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 Per-03-Q1b1x1 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
SExtractor catalog cache: saved Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
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_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits exists and is non-empty
wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (1st reference image)
verification OK: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:00.727 +45:59:45.06 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits (1st new image)
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
Image size: 944.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:47:56.593 +46:00:17.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:47:56.593 +46:00:17.20
Angular distance between the image centers 0.0149 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits (2nd new image)
verification OK: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
Image size: 944.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:47:59.615 +46:00:10.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:47:59.615 +46:00:10.36
Angular distance between the image centers 0.0077 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 04:47:56.593 +46:00:17.20
Second-epoch second image center 04:47:59.615 +46:00:10.36
Angular distance between the image centers 0.00895 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.0TaH6AvZaW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.5r6yP1Y0uW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits &> /tmp/tmp.u2QhyYpzPO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits &> /tmp/tmp.q0VhNJN34i
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.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_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.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_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Found non-empty wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
The reference image (wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits) and catalog (wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat) found
'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat' -> 'wcsmag.cat'
Read 195814 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9096 to 84.6822 deg, Dec +39.9252 to +51.3404 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 59.9096 to 84.6822 deg, Dec 39.9252 to 51.3404 deg
Loaded 12199 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): 6231 out of 9378 total matches.
Matched with Tycho-2 9378 out of 195814 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.807400
a=0.000000 b=1.000000 c=22.807400
From vast_summary.log: estimated ref. image limiting mag.: -7.37
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 195814 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9096 to 84.6822 deg, Dec +39.9252 to +51.3404 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 59.9096 to 84.6822 deg, Dec 39.9252 to 51.3404 deg
Loaded 12199 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): 6231 out of 9378 total matches.
Matched with Tycho-2 9378 out of 195814 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Forced-photometry filter: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -> calib.txt_param_ref_wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (aperture=4.5)
Read 196080 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9097 to 84.6518 deg, Dec +39.9253 to +51.3374 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 59.9097 to 84.6518 deg, Dec 39.9253 to 51.3374 deg
Loaded 12186 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): 6203 out of 9379 total matches.
Matched with Tycho-2 9379 out of 196080 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Forced-photometry filter: calibrated wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -> calib.txt_param_ref_wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 54 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
1.9 pix Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
2.7 pix fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
2.6 pix fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
Limiting magnitude estimates:
15.4 mag. Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
15.4 mag. Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
13.2 mag. fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
13.2 mag. fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.0TaH6AvZaW (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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=57, blended=26966, bad_region=1, passed=195757
Got 195757 stars (including 168489 good ones) from the SExtractor catalog wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
util/solve_plate_with_UCAC5 got 195757 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 4885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 195757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 195757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 195757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4885 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits N_match=4885 sigma_overall_arcsec=0.425 sigma_q1_arcsec=0.549 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.426 sigma_q4_arcsec=0.329 n_q1=1093 n_q2=1064 n_q3=1516 n_q4=1212 worst_quadrant_to_overall_ratio=1.293
The image catalog is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.5r6yP1Y0uW (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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=67, blended=27081, bad_region=0, passed=196013
Got 196013 stars (including 168638 good ones) from the SExtractor catalog wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
util/solve_plate_with_UCAC5 got 196013 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 4877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 196013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 196013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 196013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4877 stars left (next iteration limit 5364)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits N_match=4877 sigma_overall_arcsec=0.435 sigma_q1_arcsec=0.573 sigma_q2_arcsec=0.418 sigma_q3_arcsec=0.426 sigma_q4_arcsec=0.344 n_q1=1089 n_q2=1072 n_q3=1507 n_q4=1209 worst_quadrant_to_overall_ratio=1.318
The image catalog is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.u2QhyYpzPO (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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
WCS-calibrated image found: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
Checking if the catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
WCS catalog name: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=1166, bad_region=0, passed=31899
Got 31899 stars (including 30680 good ones) from the SExtractor catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat
util/solve_plate_with_UCAC5 got 31899 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 4856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 31856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 31856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 31856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4861 stars left (next iteration limit 5346)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4861 robust_rms=8.337 arcsec worst_quadrant_rms=13.666 arcsec
SIP_REFIT: SIP order 3 trial: matched=4861 robust_rms=0.778 arcsec worst_quadrant_rms=1.382 arcsec
SIP_REFIT: SIP order 5 trial: matched=4861 robust_rms=0.646 arcsec worst_quadrant_rms=0.991 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4861 robust_rms_before=1.401 arcsec robust_rms_before_corrected=0.564 arcsec robust_rms_after=0.646 arcsec worst_quadrant_rms_before=0.884 worst_quadrant_rms_after=0.991
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.884 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits N_match=4861 sigma_overall_arcsec=0.550 sigma_q1_arcsec=0.519 sigma_q2_arcsec=0.848 sigma_q3_arcsec=0.388 sigma_q4_arcsec=0.655 n_q1=1384 n_q2=946 n_q3=1455 n_q4=1076 worst_quadrant_to_overall_ratio=1.542
The image catalog is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits -region wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.q0VhNJN34i (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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
WCS-calibrated image found: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
Checking if the catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat corresponding to the image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
WCS catalog name: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=1105, bad_region=0, passed=32035
Got 32035 stars (including 30894 good ones) from the SExtractor catalog wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat
util/solve_plate_with_UCAC5 got 32035 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 4860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 32005 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 32005 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 32005 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4859 stars left (next iteration limit 5344)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4859 robust_rms=8.269 arcsec worst_quadrant_rms=11.638 arcsec
SIP_REFIT: SIP order 3 trial: matched=4859 robust_rms=0.777 arcsec worst_quadrant_rms=1.184 arcsec
SIP_REFIT: SIP order 5 trial: matched=4859 robust_rms=0.624 arcsec worst_quadrant_rms=1.001 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4859 robust_rms_before=1.424 arcsec robust_rms_before_corrected=0.568 arcsec robust_rms_after=0.624 arcsec worst_quadrant_rms_before=0.867 worst_quadrant_rms_after=1.001
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.867 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits N_match=4859 sigma_overall_arcsec=0.560 sigma_q1_arcsec=0.510 sigma_q2_arcsec=0.868 sigma_q3_arcsec=0.415 sigma_q4_arcsec=0.632 n_q1=1385 n_q2=983 n_q3=1410 n_q4=1081 worst_quadrant_to_overall_ratio=1.550
The image catalog is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits -region wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-06_20.00sec_0.00C_LIGHTs_0228.fits
Saving fully-calibrated image wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.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_2026-09-01_CI_Per-03-Q1b1x1_010143_TTUQ1b1x1_3658928_gzyBAmuy/wcs_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229.fits
Preparing the HTML report for the field Per-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:03:58.36 +48:38:36.1: 12.63 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:15:20.20 +49:48:52.1: 12.16 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:34:57.33 +46:27:47.1: 13.03 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:40:18.07 +51:05:32.3: 12.79 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:15:20.20 +49:48:52.1: 12.18 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:34:57.33 +46:27:47.1: 13.00 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:03:58.36 +48:38:36.1: 12.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 05:15:20.20 +49:48:52.1: ref_mag=12.17 +/- 0.01 new_mean_mag=12.0485 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter REJECTED candidate at 04:03:58.36 +48:38:36.1: ref_mag=12.62 +/- 0.02 new_mean_mag=12.3925 delta=0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:34:57.33 +46:27:47.1: ref_mag=13.02 +/- 0.01 new_mean_mag=12.7721 delta=0.24 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:40:18.07 +51:05:32.3: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Forced photometry filter REJECTED candidate at 04:40:18.07 +51:05:32.3: ref_mag=12.75 +/- 0.02 new_mean_mag=12.4712 delta=0.28 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:49:53.47 +49:03:28.6: 13.26 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:20:28.86 +45:50:16.1: 13.26 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:49:53.47 +49:03:28.6: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 04:49:53.47 +49:03:28.6: ref_mag=13.28 +/- 0.02 new_mean_mag=12.3378 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:20:28.86 +45:50:16.1: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 04:20:28.86 +45:50:16.1: ref_mag=13.23 +/- 0.02 new_mean_mag=12.3261 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:37:47.91 +42:27:40.1: 12.90 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:37:47.91 +42:27:40.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter KEPT candidate at 04:37:47.91 +42:27:40.1: ref_mag=12.92 +/- 0.02 new_mean_mag=11.9808 delta=0.93 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:38:32.01 +42:28:05.1: 12.63 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:40:30.28 +43:11:52.4: 12.11 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:38:32.01 +42:28:05.1: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:53:15.55 +41:48:57.0: 11.45 +/- 0.01 detection
Forced photometry filter KEPT candidate at 04:38:32.01 +42:28:05.1: ref_mag=12.60 +/- 0.01 new_mean_mag=11.6336 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:40:30.28 +43:11:52.4: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter KEPT candidate at 04:40:30.28 +43:11:52.4: ref_mag=12.12 +/- 0.01 new_mean_mag=11.1483 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-03-Q1b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:53:15.55 +41:48:57.0: 11.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.00
Forced photometry filter KEPT candidate at 04:53:15.55 +41:48:57.0: ref_mag=11.43 +/- 0.00 new_mean_mag=10.4887 delta=0.94 (need > 0.90)
Adding exclusion_list_local.txt__out145470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91873.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223900_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 223900_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223905_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 223905_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:11:04.18 +45:12:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223906_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 223906_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223907_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 223907_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:19:01.50 +49:19:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223909_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 223909_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:06:47.82 +44:40:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223969_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 223969_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:06:26.12 +41:15:18.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 223970_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 223970_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:33:24.31 +43:05:03.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 223972_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 223972_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:23:59.73 +41:56:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223995_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 223995_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
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Considering the candidate 223999_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 223999_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:43:32.00 +49:59:19.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 224007_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 224007_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:16:39.55 +45:38:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224037_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 224037_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:42:52.46 +43:23:13.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 224038_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 224038_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
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Considering the candidate 224041_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 224041_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:18:04.13 +45:37:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224047_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 224047_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:06:37.11 +46:13:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224073_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 224073_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:17:16.00 +46:11:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224121_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 224121_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:15:09.61 +50:40:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224199_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 224199_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:22:57.95 +49:34:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45279_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 45279_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:55:23.74 +48:21:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21434_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 21434_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:25:56.34 +49:53:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02961_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 02961_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:22:38.12 +51:05:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137026_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 137026_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:43:26.72 +43:32:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69840_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 69840_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:44:41.92 +47:04:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165825_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 165825_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:42:28.70 +41:32:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92302_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 92302_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:50:00.97 +45:46:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25749_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 25749_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:21:35.47 +49:37:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72032_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 72032_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
Rejecting candidate due to large distance (30.9") between the two second-epoch detections
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Considering the candidate 170520_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 170520_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:43:16.42 +41:43:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97808_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 97808_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:14:34.85 +45:05:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91873_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
Preparing report for the candidate 91873_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
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Considering the candidate 34457_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
Preparing report for the candidate 34457_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
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Considering the candidate 138372_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 138372_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:39:20.38 +43:29:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156863_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 156863_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:09:44.60 +40:44:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57751_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 57751_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:59:15.31 +47:36:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59241_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 59241_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:02:33.05 +47:27:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16061_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 16061_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:25:28.80 +50:14:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93325_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 93325_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:52:33.43 +45:41:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185318_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
Preparing report for the candidate 185318_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
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Considering the candidate 170083_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 170083_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:27:32.45 +41:47:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93636_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 93636_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:22:42.61 +45:07:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06844_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 06844_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:27:03.83 +50:07:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164474_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 164474_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:48:08.02 +41:26:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175155_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 175155_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:12:31.81 +41:34:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185020_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
Preparing report for the candidate 185020_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
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Considering the candidate 40742_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 40742_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:12:19.75 +48:40:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145470_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
Preparing report for the candidate 145470_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
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Considering the candidate 60260_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 60260_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:48:11.53 +47:38:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183613_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 183613_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:07:58.04 +42:13:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173081_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
Preparing report for the candidate 173081_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
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Considering the candidate 95776_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 95776_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:32:36.75 +45:40:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21271_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 21271_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 04:54:15.08 +49:53:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145826_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 145826_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:02:28.61 +41:04:33.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 145464_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 145464_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
**** FOUND 05:18:15.45 +42:47:31.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 161730_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229
The candidate 161730_fd_Per-03-Q1b1x1_2026-09-01_01-00-56_20.00sec_-0.00C_LIGHTs_0229 did not pass the final checks
