This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 25.2838 2461185.7838 12.98 15:47:59.35 +07:34:51.5
16.24177 43.89102 galactic Ser Second-epoch detections are separated by 0.5" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.304 Olga 2 -1 3 13.3 0 0
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:47:59.35 +07:34:51.5: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:47:59.35 +07:34:51.5: 16.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 25.2838* 15 47 59.35 +07 34 51.5 13.0 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461185.7838,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260525.2838 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.2838 2461185.7838 13.16 15:10:17.14 +06:32:59.3
7.34746 51.15361 galactic Vir Second-epoch detections are separated by 0.7" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.472 Roma 2 -1 2 13.1 -0 0
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:10:17.14 +06:32:59.3: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:10:17.14 +06:32:59.3: 16.17 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 25.2838* 15 10 17.14 +06 32 59.3 13.2 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461185.7838,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260525.2838 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.2838 2461185.7838 12.25 15:35:29.44 +01:54:44.0
7.33629 43.34499 galactic Ser Second-epoch detections are separated by 0.6" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.173 Ino 2 -1 2 12.6 0 0
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:35:29.44 +01:54:44.0: 13.82 +/- 0.05 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:35:29.44 +01:54:44.0: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 25.2838* 15 35 29.44 +01 54 44.0 12.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461185.7838,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260525.2838 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.2838 2461185.7838 13.54 15:27:23.60 +04:28:28.7
8.57946 46.48765 galactic Ser Second-epoch detections are separated by 1.4" and 9.2 pix
The object was found in VSX 1" V0347 Ser
Type: SR:
# Max. Min./Amp. JD0 Period
12.900 V 15.000 V 448.000000000000 C(N)
The object was not found in astcheck.
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:27:23.60 +04:28:28.7: 14.39 +/- 0.07 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:27:23.60 +04:28:28.7: 14.55 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 25.2838* 15 27 23.60 +04 28 28.7 13.5 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0347 Ser,2461185.7838,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0347 Ser 20260525.2838 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.2838 2461185.7838 12.40 15:29:11.63 +06:08:31.3
10.95330 47.06954 galactic Ser Second-epoch detections are separated by 0.3" and 9.2 pix
The object was found in VSX 1" NSVS 13436485
Type: RRAB
# Max. Min./Amp. JD0 Period
13.125 CV Y 0.870 CV 2453467.16980 0.542298500000
The object was not found in astcheck.
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:29:11.63 +06:08:31.3: 13.30 +/- 0.03 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:29:11.63 +06:08:31.3: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 05 25.2838* 15 29 11.63 +06 08 31.3 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13436485,2461185.7838,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13436485 20260525.2838 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461120.98298340 21.03.2026 11:35:19.766 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
First image: 2461120.98298340 21.03.2026 11:35:19.766 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Last image: 2461185.78408520 25.05.2026 06:48:54.961 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6600
Objects passed selection criteria: 6593
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 5876
Average stars matched: 5797.75 (98.6683 %)
Memory usage VmPeak: 113116 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 02:02:15 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461120.98298340 21.03.2026 11:35:19.766 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
First image: 2461120.98298340 21.03.2026 11:35:19.766 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Last image: 2461185.78408520 25.05.2026 06:48:54.961 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 43
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 39760
Objects passed selection criteria: 39686
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 36455
Average stars matched: 35253.5 (96.7042 %)
Memory usage VmPeak: 144204 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 02:03:48 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat to cache
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.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: 2461185.78350888
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits exists and is non-empty
Saving wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits to local_wcs_cache/
'wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits' -> 'local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits'
wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits exists and is non-empty
Saving wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits to local_wcs_cache/
'wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits' -> 'local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits'
wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits exists and is non-empty
Saving wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits to local_wcs_cache/
'wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits' -> 'local_wcs_cache/wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits'
wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits exists and is non-empty
Saving wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits to local_wcs_cache/
'wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits' -> 'local_wcs_cache/wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits (1st reference image)
verification OK: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:45.434 +05:59:44.20 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits (1st new image)
verification OK: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:42.950 +06:00:12.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:45.434 +05:59:44.20
Second-epoch image center 15:25:42.950 +06:00:12.10
Angular distance between the image centers 0.0129 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits (2nd new image)
verification OK: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:39.964 +05:59:39.82 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:45.434 +05:59:44.20
Second-epoch image center 15:25:39.964 +05:59:39.82
Angular distance between the image centers 0.0227 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 15:25:42.950 +06:00:12.10
Second-epoch second image center 15:25:39.964 +05:59:39.82
Angular distance between the image centers 0.01528 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits &> /tmp/tmp.zQfH1M1447
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits &> /tmp/tmp.Bu3glho9Xp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits &> /tmp/tmp.DYipZ1QLPn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits &> /tmp/tmp.2FmmXwW53o
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
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_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
Found non-empty wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
The reference image (wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits) and catalog (wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat) found
'wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat' -> 'wcsmag.cat'
Read 8926 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5451 to 239.4424 deg, Dec +0.6561 to +11.2816 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 223.5451 to 239.4424 deg, Dec 0.6561 to 11.2816 deg
Loaded 4656 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3898 out of 4076 total matches.
Matched with Tycho-2 4076 out of 8926 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.928400
a=0.000000 b=1.000000 c=22.928400
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8926 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5451 to 239.4424 deg, Dec +0.6561 to +11.2816 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 223.5451 to 239.4424 deg, Dec 0.6561 to 11.2816 deg
Loaded 4656 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3898 out of 4076 total matches.
Matched with Tycho-2 4076 out of 8926 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits (aperture=6.4)
Read 8697 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5431 to 239.4424 deg, Dec +0.6252 to +11.2700 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 223.5431 to 239.4424 deg, Dec 0.6252 to 11.2700 deg
Loaded 4669 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3846 out of 4063 total matches.
Matched with Tycho-2 4063 out of 8697 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
2.3 pix Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
2.3 pix fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
2.3 pix fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
2.4 pix wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
2.3 pix wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Limiting magnitude estimates:
15.3 mag. Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
15.3 mag. Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
14.8 mag. fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
14.8 mag. fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zQfH1M1447 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits' -> 'wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=521, passed=8926
Got 8926 stars (including 8397 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
util/solve_plate_with_UCAC5 got 8926 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 8798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits N_match=974 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.490 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.411 n_q1=272 n_q2=235 n_q3=251 n_q4=216 worst_quadrant_to_overall_ratio=1.305
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits -region wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Bu3glho9Xp (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits' -> 'wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=573, passed=8695
Got 8695 stars (including 8117 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat
util/solve_plate_with_UCAC5 got 8695 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 8555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 8555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 8555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits N_match=973 sigma_overall_arcsec=0.451 sigma_q1_arcsec=0.370 sigma_q2_arcsec=0.549 sigma_q3_arcsec=0.427 sigma_q4_arcsec=0.486 n_q1=273 n_q2=245 n_q3=243 n_q4=212 worst_quadrant_to_overall_ratio=1.217
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits -region wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DYipZ1QLPn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
WCS_IMAGE_NAME=wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
WCS-calibrated image found: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
Checking if the catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
WCS catalog name: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=397, passed=6039
Got 6039 stars (including 5638 good ones) from the SExtractor catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat
util/solve_plate_with_UCAC5 got 6039 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5989 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5989 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits N_match=976 sigma_overall_arcsec=0.444 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.588 sigma_q3_arcsec=0.386 sigma_q4_arcsec=0.619 n_q1=267 n_q2=238 n_q3=257 n_q4=214 worst_quadrant_to_overall_ratio=1.395
The image catalog is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits -region wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2FmmXwW53o (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
Checking if the catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
WCS catalog name: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=404, passed=6094
Got 6094 stars (including 5688 good ones) from the SExtractor catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat
util/solve_plate_with_UCAC5 got 6094 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 6042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 6042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 6042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits N_match=975 sigma_overall_arcsec=0.401 sigma_q1_arcsec=0.292 sigma_q2_arcsec=0.576 sigma_q3_arcsec=0.335 sigma_q4_arcsec=0.555 n_q1=269 n_q2=236 n_q3=257 n_q4=213 worst_quadrant_to_overall_ratio=1.437
The image catalog is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits -region wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits sigma_overall=0.376 worst_q_ratio=1.305
ref2=Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits sigma_overall=0.451 worst_q_ratio=1.217
new1=fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits sigma_overall=0.444 worst_q_ratio=1.395
new2=fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits sigma_overall=0.401 worst_q_ratio=1.437
reference average sigma_overall=0.4135 worst_q_ratio=1.261
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532_astrometric_residuals.png (974 matched stars from wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533_astrometric_residuals.png (973 matched stars from wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254_astrometric_residuals.png (976 matched stars from wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255_astrometric_residuals.png (975 matched stars from wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits'
Saving fully-calibrated image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits'
Preparing the HTML report for the field Ser-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:40:22.98 +02:37:14.1: 11.39 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:40:22.98 +02:37:14.1: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.00
Forced photometry filter REJECTED candidate at 15:40:22.98 +02:37:14.1: ref_mag=11.42 +/- 0.00 new_mean_mag=11.6397 delta=-0.22 (need > 0.90)
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 20280_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 20280_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20287_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 20287_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:18:42.65 +02:07:30.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20289_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 20289_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:18:39.69 +02:07:17.3 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 Ser-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat to cache
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Creating symlink local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits exists and is non-empty
wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits exists and is non-empty
wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits exists and is non-empty
wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits (1st reference image)
verification OK: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:45.434 +05:59:44.20 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits (1st new image)
verification OK: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:42.950 +06:00:12.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:45.434 +05:59:44.20
Second-epoch image center 15:25:42.950 +06:00:12.10
Angular distance between the image centers 0.0129 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits (2nd new image)
verification OK: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:25:39.964 +05:59:39.82 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:45.434 +05:59:44.20
Second-epoch image center 15:25:39.964 +05:59:39.82
Angular distance between the image centers 0.0227 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 15:25:42.950 +06:00:12.10
Second-epoch second image center 15:25:39.964 +05:59:39.82
Angular distance between the image centers 0.01528 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits &> /tmp/tmp.OcLR0NrLLj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits &> /tmp/tmp.QWkXoqAP70
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits &> /tmp/tmp.cyI9s0kbp0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits &> /tmp/tmp.dO4mQ0dtT2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
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_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
Found non-empty wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits and wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
The reference image (wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits) and catalog (wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat) found
'wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat' -> 'wcsmag.cat'
Read 50422 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5430 to 239.4714 deg, Dec +0.6305 to +11.2886 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 223.5430 to 239.4714 deg, Dec 0.6305 to 11.2886 deg
Loaded 4685 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3662 out of 4090 total matches.
Matched with Tycho-2 4090 out of 50422 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.812400
a=0.000000 b=1.000000 c=22.812400
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 50422 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5430 to 239.4714 deg, Dec +0.6305 to +11.2886 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 223.5430 to 239.4714 deg, Dec 0.6305 to 11.2886 deg
Loaded 4685 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3662 out of 4090 total matches.
Matched with Tycho-2 4090 out of 50422 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits (aperture=5.0)
Read 51564 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.5411 to 239.4698 deg, Dec +0.6229 to +11.2765 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 223.5411 to 239.4698 deg, Dec 0.6229 to 11.2765 deg
Loaded 4682 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3631 out of 4069 total matches.
Matched with Tycho-2 4069 out of 51564 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 34 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
2.1 pix Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
2.2 pix fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
2.3 pix fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
2.3 pix wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
2.1 pix wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Limiting magnitude estimates:
15.5 mag. Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
15.5 mag. Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
15.0 mag. fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
15.0 mag. fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OcLR0NrLLj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits' -> 'wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2486, passed=50406
Got 50406 stars (including 47846 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat
util/solve_plate_with_UCAC5 got 50406 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 49664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 49665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 49664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits N_match=973 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.302 sigma_q2_arcsec=0.479 sigma_q3_arcsec=0.382 sigma_q4_arcsec=0.450 n_q1=272 n_q2=246 n_q3=234 n_q4=221 worst_quadrant_to_overall_ratio=1.229
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits -region wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QWkXoqAP70 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits' -> 'wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat corresponding to the image wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2509, passed=51546
Got 51546 stars (including 48975 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat
util/solve_plate_with_UCAC5 got 51546 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 50857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 50857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 50856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits N_match=974 sigma_overall_arcsec=0.450 sigma_q1_arcsec=0.364 sigma_q2_arcsec=0.562 sigma_q3_arcsec=0.443 sigma_q4_arcsec=0.495 n_q1=268 n_q2=253 n_q3=233 n_q4=220 worst_quadrant_to_overall_ratio=1.249
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits -region wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cyI9s0kbp0 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
WCS_IMAGE_NAME=wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
WCS-calibrated image found: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
Checking if the catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
WCS catalog name: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1705, passed=35259
Got 35259 stars (including 33501 good ones) from the SExtractor catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat
util/solve_plate_with_UCAC5 got 35259 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 34726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 34727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 34727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits N_match=975 sigma_overall_arcsec=0.433 sigma_q1_arcsec=0.344 sigma_q2_arcsec=0.583 sigma_q3_arcsec=0.363 sigma_q4_arcsec=0.577 n_q1=274 n_q2=234 n_q3=261 n_q4=206 worst_quadrant_to_overall_ratio=1.345
The image catalog is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits -region wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dO4mQ0dtT2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
Checking if the catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat corresponding to the image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
WCS catalog name: wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1639, passed=35022
Got 35022 stars (including 33335 good ones) from the SExtractor catalog wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat
util/solve_plate_with_UCAC5 got 35022 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 34534 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 34533 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 34533 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits N_match=975 sigma_overall_arcsec=0.386 sigma_q1_arcsec=0.290 sigma_q2_arcsec=0.548 sigma_q3_arcsec=0.313 sigma_q4_arcsec=0.528 n_q1=275 n_q2=234 n_q3=258 n_q4=208 worst_quadrant_to_overall_ratio=1.418
The image catalog is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits -region wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-05_20.00sec_5.00C_LIGHT_0254.fits
Saving fully-calibrated image wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Ser-03-Q2b1x1_020001_TTUQ2b1x1_2508270_WcxoB2Hg/wcs_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255.fits
Preparing the HTML report for the field Ser-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:47:59.35 +07:34:51.5: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:26:44.39 +03:20:34.6: 14.67 +/- 0.10 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:40:22.96 +02:37:14.0: 11.64 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:47:03.73 +02:23:44.0: 13.89 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:10:17.14 +06:32:59.3: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:41:53.27 +04:59:50.4: 14.32 +/- 0.08 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:43:29.84 +03:51:05.5: 12.93 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:36:24.84 +02:56:15.9: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:47:03.73 +02:23:44.0: 13.98 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:26:44.39 +03:20:34.6: 14.46 +/- 0.07 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:43:29.84 +03:51:05.5: 13.06 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:10:17.14 +06:32:59.3: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:47:59.35 +07:34:51.5: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:41:53.27 +04:59:50.4: 14.21 +/- 0.07 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:36:24.84 +02:56:15.9: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:40:22.96 +02:37:14.0: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry reference-image weighted average: 14.53 +/- 0.06
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter REJECTED candidate at 15:26:44.39 +03:20:34.6: ref_mag=14.53 +/- 0.06 new_mean_mag=14.7752 delta=-0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:47:03.73 +02:23:44.0: ref_mag=13.93 +/- 0.04 new_mean_mag=14.1451 delta=-0.21 (need > 0.90)
Forced photometry reference-image weighted average: 14.26 +/- 0.05
Forced photometry filter REJECTED candidate at 15:43:29.84 +03:51:05.5: ref_mag=12.99 +/- 0.02 new_mean_mag=13.1419 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Forced photometry filter REJECTED candidate at 15:41:53.27 +04:59:50.4: ref_mag=14.26 +/- 0.05 new_mean_mag=14.5407 delta=-0.28 (need > 0.90)
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter REJECTED candidate at 15:40:22.96 +02:37:14.0: ref_mag=11.66 +/- 0.01 new_mean_mag=11.7857 delta=-0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:36:24.84 +02:56:15.9: ref_mag=12.77 +/- 0.01 new_mean_mag=12.8291 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:41:09.02 +02:55:53.1: 13.89 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:33:10.34 +03:53:21.5: 13.94 +/- 0.05 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:11:24.74 +02:33:17.0: 13.95 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:49:55.26 +02:48:51.0: 13.78 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:48:24.92 +06:38:57.5: 13.92 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:45:47.49 +05:35:54.7: 14.49 +/- 0.10 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:41:09.02 +02:55:53.1: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Forced photometry filter REJECTED candidate at 15:41:09.02 +02:55:53.1: ref_mag=13.92 +/- 0.04 new_mean_mag=13.9751 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:39:41.37 +09:59:49.3: 14.20 +/- 0.08 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:33:10.34 +03:53:21.5: 13.95 +/- 0.05 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:49:55.26 +02:48:51.0: 13.80 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:48:24.92 +06:38:57.5: 14.00 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:11:24.74 +02:33:17.0: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter REJECTED candidate at 15:33:10.34 +03:53:21.5: ref_mag=13.95 +/- 0.04 new_mean_mag=14.0595 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:49:55.26 +02:48:51.0: ref_mag=13.79 +/- 0.04 new_mean_mag=14.0494 delta=-0.26 (need > 0.90)
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter REJECTED candidate at 15:11:24.74 +02:33:17.0: ref_mag=13.93 +/- 0.04 new_mean_mag=14.0521 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:48:24.92 +06:38:57.5: ref_mag=13.96 +/- 0.04 new_mean_mag=14.2707 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:45:47.49 +05:35:54.7: 14.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.06
Forced photometry filter REJECTED candidate at 15:45:47.49 +05:35:54.7: ref_mag=14.33 +/- 0.06 new_mean_mag=14.4413 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:44:17.71 +02:37:59.3: 15.32 +/- 0.22 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:39:41.37 +09:59:49.3: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Forced photometry filter REJECTED candidate at 15:39:41.37 +09:59:49.3: ref_mag=14.13 +/- 0.05 new_mean_mag=14.1919 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:39:44.93 +03:45:25.5: 14.49 +/- 0.10 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:44:17.71 +02:37:59.3: 14.83 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.11
Forced photometry filter REJECTED candidate at 15:44:17.71 +02:37:59.3: ref_mag=14.96 +/- 0.11 new_mean_mag=14.8432 delta=0.12 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:49:09.83 +02:18:51.7: 15.11 +/- 0.18 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:38:02.47 +04:26:25.2: 14.61 +/- 0.10 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:46:36.58 +05:19:31.6: 15.54 +/- 0.23 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:48:52.57 +06:56:24.7: 15.35 +/- 0.21 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:35:29.44 +01:54:44.0: 13.82 +/- 0.05 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:39:44.93 +03:45:25.5: 14.38 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.07
Forced photometry filter REJECTED candidate at 15:39:44.93 +03:45:25.5: ref_mag=14.43 +/- 0.07 new_mean_mag=14.5958 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:38:02.47 +04:26:25.2: 14.56 +/- 0.09 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:49:09.83 +02:18:51.7: 15.45 +/- 0.25 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:46:36.58 +05:19:31.6: 15.28 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.07
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:48:52.57 +06:56:24.7: 15.15 +/- 0.17 detection
Forced photometry filter REJECTED candidate at 15:38:02.47 +04:26:25.2: ref_mag=14.58 +/- 0.07 new_mean_mag=14.8529 delta=-0.27 (need > 0.90)
Forced photometry reference-image weighted average: 15.23 +/- 0.15
Forced photometry reference-image weighted average: 15.38 +/- 0.15
Forced photometry filter REJECTED candidate at 15:49:09.83 +02:18:51.7: ref_mag=15.23 +/- 0.15 new_mean_mag=14.7381 delta=0.49 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:46:36.58 +05:19:31.6: ref_mag=15.38 +/- 0.15 new_mean_mag=14.9377 delta=0.44 (need > 0.90)
Forced photometry reference-image weighted average: 15.23 +/- 0.13
Forced photometry filter REJECTED candidate at 15:48:52.57 +06:56:24.7: ref_mag=15.23 +/- 0.13 new_mean_mag=14.8458 delta=0.38 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:27:23.60 +04:28:28.7: 14.39 +/- 0.07 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:35:29.44 +01:54:44.0: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 15:35:29.44 +01:54:44.0: ref_mag=13.81 +/- 0.03 new_mean_mag=12.2538 delta=1.56 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:27:23.60 +04:28:28.7: 14.55 +/- 0.08 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-35-19_20.00sec_-14.90C_LIGHT_0532.fits at 15:29:11.63 +06:08:31.3: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.05
Forced photometry filter KEPT candidate at 15:27:23.60 +04:28:28.7: ref_mag=14.46 +/- 0.05 new_mean_mag=13.5396 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-03-21_06-36-12_20.00sec_-15.00C_LIGHT_0533.fits at 15:29:11.63 +06:08:31.3: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 15:29:11.63 +06:08:31.3: ref_mag=13.32 +/- 0.02 new_mean_mag=12.4039 delta=0.92 (need > 0.90)
Adding exclusion_list_local.txt__out24012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64764.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 64649_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64649_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64651_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64651_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64657_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64657_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64692_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64692_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64734_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64734_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64745_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
Preparing report for the candidate 64745_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
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Considering the candidate 64751_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64751_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:50:22.51 +02:13:06.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 64753_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64753_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64761_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64761_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:45:17.96 +05:25:38.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 64764_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
Preparing report for the candidate 64764_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
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Considering the candidate 64776_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64776_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:44:08.45 +08:06:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64780_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64780_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:26:47.99 +05:12:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64793_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64793_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:41:06.45 +09:16:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64813_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64813_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:29:09.53 +03:03:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64816_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64816_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:42:25.31 +03:19:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64831_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64831_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64836_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64836_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:44:37.34 +05:03:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64838_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64838_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64841_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64841_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64864_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64864_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64887_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64887_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:42:58.60 +06:55:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64898_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64898_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64900_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64900_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64908_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64908_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64957_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64957_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 15:35:33.64 +10:13:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64961_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64961_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64964_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64964_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64971_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64971_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64978_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64978_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64979_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64979_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks
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Considering the candidate 64998_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255
The candidate 64998_fd_Ser-03-Q2b1x1_2026-05-25_01-48-54_20.00sec_5.00C_LIGHT_0255 did not pass the final checks