This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 03.2066 2461163.7066 10.16 10:06:46.58 +04:18:04.8
235.70487 44.61237 galactic Sex Second-epoch detections are separated by 0.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.7 Iris -2 1 2 10.5 0 -0
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:06:46.58 +04:18:04.8: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:06:46.58 +04:18:04.8: 15.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.2066* 10 06 46.58 +04 18 04.8 10.2 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461163.7066,10.16,0.05,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 20260503.2066 10.16CV 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 03.2066 2461163.7066 12.46 10:30:40.68 +02:32:32.6
242.96267 48.31822 galactic Sex Second-epoch detections are separated by 1.3" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.88 Thisbe -2 1 2 12.6 0 -0
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:30:40.68 +02:32:32.6: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:30:40.68 +02:32:32.6: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.2066* 10 30 40.68 +02 32 32.6 12.5 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461163.7066,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260503.2066 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2066 2461163.7066 12.88 10:23:08.92 +09:17:34.7
232.82944 50.75188 galactic Leo Second-epoch detections are separated by 0.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.35 Leukothea -1 1 2 13.0 -0 0
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:23:08.92 +09:17:34.7: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:23:08.92 +09:17:34.7: 16.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.2066* 10 23 08.92 +09 17 34.7 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461163.7066,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260503.2066 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2066 2461163.7066 13.25 10:38:19.88 +08:00:38.2
237.94171 53.16274 galactic Leo Second-epoch detections are separated by 1.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.356 Liguria -0 1 1 13.2 0 -0
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:38:19.88 +08:00:38.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:38:19.88 +08:00:38.2: 15.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.2066* 10 38 19.88 +08 00 38.2 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461163.7066,13.25,0.05,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 20260503.2066 13.25CV 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 03.2066 2461163.7066 13.46 10:11:22.90 +07:44:47.9
232.46939 47.46569 galactic Leo Second-epoch detections are separated by 1.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.554 Peraga -2 1 2 13.8 0 0
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:11:22.90 +07:44:47.9: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:11:22.90 +07:44:47.9: 16.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.2066* 10 11 22.90 +07 44 47.9 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461163.7066,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260503.2066 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.2066 2461163.7066 13.65 10:13:46.28 +04:11:40.3
237.25481 45.97774 galactic Sex Second-epoch detections are separated by 0.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.336 Lacadiera -1 1 1 13.9 0 -0
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:13:46.28 +04:11:40.3: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:13:46.28 +04:11:40.3: 16.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.2066* 10 13 46.28 +04 11 40.3 13.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461163.7066,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260503.2066 13.65CV 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: 2461146.71049043 16.04.2026 05:02:56.373 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
First image: 2461146.71049043 16.04.2026 05:02:56.373 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
Last image: 2461163.70690634 03.05.2026 04:57:46.708 /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
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: 2 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): 4625
Objects passed selection criteria: 4619
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 3920.5
Average stars matched: 3797.5 (96.8626 %)
Memory usage VmPeak: 111408 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 00:01:32 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.71049043 16.04.2026 05:02:56.373 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
First image: 2461146.71049043 16.04.2026 05:02:56.373 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
Last image: 2461163.70690634 03.05.2026 04:57:46.708 /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 26677
Objects passed selection criteria: 26612
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 23496.5
Average stars matched: 22432.2 (95.4706 %)
Memory usage VmPeak: 133212 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 00:02:46 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/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
SExtractor catalog cache: saved Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat to cache
SExtractor catalog cache: saved Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.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/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461163.70622133
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_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits exists and is non-empty
Saving wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits to local_wcs_cache/
'wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits' -> 'local_wcs_cache/wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits'
wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits exists and is non-empty
Saving wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits to local_wcs_cache/
'wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits' -> 'local_wcs_cache/wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits'
wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits exists and is non-empty
Saving wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits to local_wcs_cache/
'wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits' -> 'local_wcs_cache/wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits'
wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits exists and is non-empty
Saving wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits to local_wcs_cache/
'wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits' -> 'local_wcs_cache/wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits (1st reference image)
verification OK: wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:17:11.223 +05:59:22.20 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_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits (1st new image)
verification OK: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:17:11.672 +06:00:18.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:17:11.223 +05:59:22.20
Second-epoch image center 10:17:11.672 +06:00:18.57
Angular distance between the image centers 0.0158 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits (2nd new image)
verification OK: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:17:14.577 +05:59:52.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:17:11.223 +05:59:22.20
Second-epoch image center 10:17:14.577 +05:59:52.71
Angular distance between the image centers 0.0163 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 10:17:11.672 +06:00:18.57
Second-epoch second image center 10:17:14.577 +05:59:52.71
Angular distance between the image centers 0.01402 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/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits &> /tmp/tmp.cFmPy83yNp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits &> /tmp/tmp.z79n5vAZ9C
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits &> /tmp/tmp.DT4Rvw0MDZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits &> /tmp/tmp.TQeRX5thhU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat
Found non-empty wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat
The reference image (wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits) and catalog (wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat) found
'wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat' -> 'wcsmag.cat'
Read 6928 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 146.2543 to 162.2032 deg, Dec +0.5952 to +11.2921 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 146.2543 to 162.2032 deg, Dec 0.5952 to 11.2921 deg
Loaded 4744 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): 3795 out of 3932 total matches.
Matched with Tycho-2 3932 out of 6928 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.772300
a=0.000000 b=1.000000 c=22.772300
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6928 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 146.2543 to 162.2032 deg, Dec +0.5952 to +11.2921 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 146.2543 to 162.2032 deg, Dec 0.5952 to 11.2921 deg
Loaded 4744 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): 3795 out of 3932 total matches.
Matched with Tycho-2 3932 out of 6928 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits:
Forced-photometry filter: calibrated wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits -> calib.txt_param_ref_wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits (aperture=6.5)
Read 6613 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 146.1402 to 162.6215 deg, Dec +0.1984 to +11.5941 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 146.1402 to 162.6215 deg, Dec 0.1984 to 11.5941 deg
Loaded 5210 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): 3754 out of 3927 total matches.
Matched with Tycho-2 3927 out of 6613 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits:
Forced-photometry filter: calibrated wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits -> calib.txt_param_ref_wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
2.1 pix Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
2.5 pix fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
2.5 pix fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
2.5 pix wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
2.1 pix wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
Limiting magnitude estimates:
15.2 mag. Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
15.3 mag. Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
14.3 mag. fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
14.3 mag. fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.cFmPy83yNp (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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits' -> 'wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
WCS-calibrated image found: wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
Checking if the catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat corresponding to the image wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat corresponding to the image wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
WCS catalog name: wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=443, passed=6928
Got 6928 stars (including 6481 good ones) from the SExtractor catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat
util/solve_plate_with_UCAC5 got 6928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 6795 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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 6791 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 6791 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits -region wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.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.z79n5vAZ9C (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits' -> 'wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
WCS_IMAGE_NAME=wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
WCS-calibrated image found: wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
Checking if the catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat corresponding to the image wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits alredy exist and is non-empty...
Catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat corresponding to the image wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
WCS catalog name: wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=465, passed=6613
Got 6613 stars (including 6136 good ones) from the SExtractor catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat
util/solve_plate_with_UCAC5 got 6613 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 509 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 6416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 450 to 509 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 6416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 6416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits -region wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.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.DT4Rvw0MDZ (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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
WCS_IMAGE_NAME=wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
WCS-calibrated image found: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
Checking if the catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat corresponding to the image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat corresponding to the image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
WCS catalog name: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=334, passed=3813
Got 3813 stars (including 3477 good ones) from the SExtractor catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat
util/solve_plate_with_UCAC5 got 3813 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 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 3725 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 3722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 3722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits -region wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.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.TQeRX5thhU (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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
WCS_IMAGE_NAME=wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
WCS-calibrated image found: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
Checking if the catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat corresponding to the image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat corresponding to the image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
WCS catalog name: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=325, passed=3796
Got 3796 stars (including 3468 good ones) from the SExtractor catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat
util/solve_plate_with_UCAC5 got 3796 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 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 3708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 3709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 3709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits -region wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits'
Saving fully-calibrated image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits'
Preparing the HTML report for the field Sex-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:06:46.58 +04:18:04.8: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:06:46.58 +04:18:04.8: 15.90 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20489.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20489_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
Preparing report for the candidate 20489_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Sex-01-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 ####
10:06:46.58 +04:18:04.8
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/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
SExtractor catalog cache: saved Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat to cache
SExtractor catalog cache: saved Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
Creating symlink local_wcs_cache/wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
Creating symlink local_wcs_cache/wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
Creating symlink local_wcs_cache/wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.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_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits exists and is non-empty
wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits exists and is non-empty
wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits exists and is non-empty
wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits (1st reference image)
verification OK: wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:17:11.223 +05:59:22.20 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_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits (1st new image)
verification OK: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:17:11.672 +06:00:18.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:17:11.223 +05:59:22.20
Second-epoch image center 10:17:11.672 +06:00:18.57
Angular distance between the image centers 0.0158 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits (2nd new image)
verification OK: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:17:14.577 +05:59:52.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:17:11.223 +05:59:22.20
Second-epoch image center 10:17:14.577 +05:59:52.71
Angular distance between the image centers 0.0163 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 10:17:11.672 +06:00:18.57
Second-epoch second image center 10:17:14.577 +05:59:52.71
Angular distance between the image centers 0.01402 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/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits &> /tmp/tmp.xyBWYcWDhP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits &> /tmp/tmp.d6ToI4vvmC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits &> /tmp/tmp.cKJyyxUdw2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits &> /tmp/tmp.UlhC6het5j
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat
Found non-empty wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits and wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat
The reference image (wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits) and catalog (wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat) found
'wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat' -> 'wcsmag.cat'
Read 36425 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 146.2543 to 162.2045 deg, Dec +0.5952 to +11.2954 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 146.2543 to 162.2045 deg, Dec 0.5952 to 11.2954 deg
Loaded 4750 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): 3712 out of 4031 total matches.
Matched with Tycho-2 4031 out of 36425 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.642000
a=0.000000 b=1.000000 c=22.642000
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36425 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 146.2543 to 162.2045 deg, Dec +0.5952 to +11.2954 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 146.2543 to 162.2045 deg, Dec 0.5952 to 11.2954 deg
Loaded 4750 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): 3712 out of 4031 total matches.
Matched with Tycho-2 4031 out of 36425 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits:
Forced-photometry filter: calibrated wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits -> calib.txt_param_ref_wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits (aperture=5.0)
Read 39278 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 146.1293 to 162.6351 deg, Dec +0.1788 to +11.6671 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 146.1293 to 162.6351 deg, Dec 0.1788 to 11.6671 deg
Loaded 5262 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): 3705 out of 4075 total matches.
Matched with Tycho-2 4075 out of 39278 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits:
Forced-photometry filter: calibrated wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits -> calib.txt_param_ref_wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
2.0 pix Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
2.1 pix fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
2.1 pix fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
2.2 pix wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
2.0 pix wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
Limiting magnitude estimates:
15.3 mag. Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
15.4 mag. Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
14.5 mag. fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
14.5 mag. fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 14.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xyBWYcWDhP (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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits' -> 'wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
WCS-calibrated image found: wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
Checking if the catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat corresponding to the image wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat corresponding to the image wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits
WCS catalog name: wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1564, passed=36406
Got 36406 stars (including 34804 good ones) from the SExtractor catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat
util/solve_plate_with_UCAC5 got 36406 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 35901 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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 35898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 35898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits -region wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.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.d6ToI4vvmC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits' -> 'wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
WCS_IMAGE_NAME=wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
WCS-calibrated image found: wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
Checking if the catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat corresponding to the image wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits alredy exist and is non-empty...
Catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat corresponding to the image wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits
WCS catalog name: wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1637, passed=39258
Got 39258 stars (including 37533 good ones) from the SExtractor catalog wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat
util/solve_plate_with_UCAC5 got 39258 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 38411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 38411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 38411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 916 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits -region wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.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.cKJyyxUdw2 (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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
WCS_IMAGE_NAME=wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
WCS-calibrated image found: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
Checking if the catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat corresponding to the image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat corresponding to the image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
WCS catalog name: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=771, passed=22999
Got 22999 stars (including 22199 good ones) from the SExtractor catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat
util/solve_plate_with_UCAC5 got 22999 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 11.4)
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 22469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.4)
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 22468 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 22468 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits -region wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.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.UlhC6het5j (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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
WCS_IMAGE_NAME=wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
WCS-calibrated image found: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
Checking if the catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat corresponding to the image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat corresponding to the image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
WCS catalog name: wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=770, passed=22882
Got 22882 stars (including 22083 good ones) from the SExtractor catalog wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat
util/solve_plate_with_UCAC5 got 22882 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 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 22361 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 22360 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 22360 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits -region wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-56-47_20.00sec_-4.90C_LIGHT_0127.fits
Saving fully-calibrated image wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.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_2026-05-02_CI_Sex-01-Q2b1x1_235835_TTUQ2b1x1_4027544_99Jug17F/wcs_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128.fits
Preparing the HTML report for the field Sex-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:11:22.90 +07:44:47.9: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:38:19.88 +08:00:38.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:30:40.68 +02:32:32.6: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:23:08.92 +09:17:34.7: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:23:17.27 +06:36:52.0: 14.08 +/- 0.06 detection
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-02-56_20.00sec_-4.90C_LIGHT_0166.fits at 10:13:46.28 +04:11:40.3: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:23:17.27 +06:36:52.0: 14.00 +/- 0.05 detection
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:11:22.90 +07:44:47.9: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:30:40.68 +02:32:32.6: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:23:08.92 +09:17:34.7: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:38:19.88 +08:00:38.2: 15.90 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.03 +/- 0.04
Forced photometry filter REJECTED candidate at 10:23:17.27 +06:36:52.0: ref_mag=14.03 +/- 0.04 new_mean_mag=14.2233 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Sex-01-Q2b1x1_2026-04-16_00-10-57_20.00sec_-4.90C_LIGHTs_0145.fits at 10:13:46.28 +04:11:40.3: 16.08 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out54103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54142.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 54088_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
The candidate 54088_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54093_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
The candidate 54093_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128 did not pass the final checks
**** FOUND 10:06:46.58 +04:18:04.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54094_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
The candidate 54094_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128 did not pass the final checks
**** FOUND 10:00:55.86 +04:59:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54098_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
The candidate 54098_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128 did not pass the final checks
**** FOUND 10:25:20.42 +08:45:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54103_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
Preparing report for the candidate 54103_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54105_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
The candidate 54105_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128 did not pass the final checks
**** FOUND 10:25:23.17 +08:46:04.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54107_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
The candidate 54107_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128 did not pass the final checks
**** FOUND 10:41:28.08 +08:34:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54109_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
Preparing report for the candidate 54109_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54116_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
Preparing report for the candidate 54116_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54124_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
Preparing report for the candidate 54124_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54129_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
The candidate 54129_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128 did not pass the final checks
**** FOUND 10:20:22.13 +08:41:40.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54131_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
The candidate 54131_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128 did not pass the final checks
**** FOUND 10:18:37.40 +07:19:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54138_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128
The candidate 54138_fd_Sex-01-Q2b1x1_2026-05-02_23-57-46_20.00sec_-4.90C_LIGHT_0128 did not pass the final checks