This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi
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 08 28.1472 2461280.6472 12.03 18:46:44.44 -31:43:54.7
3.69119 -12.96226 galactic Sgr Second-epoch detections are separated by 1.8" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.451 Patientia 1 0 1 12.1 -0 -0
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:46:44.44 -31:43:54.7: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:46:44.44 -31:43:54.7: 14.65 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461280.6472,12.03,0.05,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 20260828.1472 12.03CV 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 08 28.1472 2461280.6472 12.06 18:26:49.04 -34:48:44.2
359.04647 -10.48450 galactic Sgr Second-epoch detections are separated by 0.5" and 4.9 pix
The object was found in VSX 1" ASASSN-V J182648.93-344844.8
Type: L
# Max. Min./Amp. JD0 Period
13.240 V 13.790 V
The object was not found in astcheck.
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:26:49.04 -34:48:44.2: 13.16 +/- 0.11 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:26:49.04 -34:48:44.2: 13.29 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.08
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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J182648.93-344844.8,2461280.6472,12.06,0.05,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
ASASSN-V J182648.93-344844.8 20260828.1472 12.06CV 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 08 28.1472 2461280.6472 12.12 19:05:22.34 -34:49:32.3
2.28362 -17.74590 galactic Sgr Second-epoch detections are separated by 2.0" and 4.6 pix
The object was found in VSX 2" FP Sgr
Type: M
# Max. Min./Amp. JD0 Period
12.000 V < 16.300 V 2452106.00000 229.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 19:05:22.34 -34:49:32.3: 13.94 +/- 0.20 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 19:05:22.34 -34:49:32.3: 14.60 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.94 +/- 0.20
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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FP Sgr,2461280.6472,12.12,0.05,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
FP Sgr 20260828.1472 12.12CV 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 08 28.1472 2461280.6472 11.36 18:33:04.17 -30:39:07.2
3.43285 -9.85600 galactic Sgr Second-epoch detections are separated by 0.8" and 5.1 pix
The object was found in VSX 3" ASAS J183304-3039.1
Type: MISC
# Max. Min./Amp. JD0 Period
8.545 Ic Y 0.484 Ic 2452717.00000 194.500000000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:33:04.17 -30:39:07.2: 12.48 +/- 0.05 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:33:04.17 -30:39:07.2: 12.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.04
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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J183304-3039.1,2461280.6472,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J183304-3039.1 20260828.1472 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.1472 2461280.6472 12.13 18:28:46.70 -30:04:38.2
3.54382 -8.77198 galactic Sgr Second-epoch detections are separated by 0.9" and 5.1 pix
The object was found in VSX 6" ASASSN-V J182846.36-300434.1
Type: L:
# Max. Min./Amp. JD0 Period
13.660 V 14.330 V
The object was not found in astcheck.
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:28:46.70 -30:04:38.2: 13.32 +/- 0.13 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:28:46.70 -30:04:38.2: 13.38 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.09
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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J182846.36-300434.1,2461280.6472,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J182846.36-300434.1 20260828.1472 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.1472 2461280.6472 10.35 18:28:26.87 -33:48:15.9
0.11798 -10.34826 galactic Sgr Second-epoch detections are separated by 0.5" and 4.9 pix
The object was found in VSX 4" ASAS J182827-3348.3
Type: MISC
# Max. Min./Amp. JD0 Period
11.670 V Y 0.820 V 2452538.40000 168.422531000000 Me
The object was not found in astcheck.
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:28:26.87 -33:48:15.9: 11.31 +/- 0.02 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:28:26.87 -33:48:15.9: 11.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J182827-3348.3,2461280.6472,10.35,0.05,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
ASAS J182827-3348.3 20260828.1472 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461229.75814948 08.07.2026 06:11:34.115 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
First image: 2461229.75814948 08.07.2026 06:11:34.115 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Last image: 2461280.64746398 28.08.2026 03:32:10.888 /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.47
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 8228
Objects passed selection criteria: 8204
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 5553.75
Average stars matched: 5254 (94.6027 %)
Memory usage VmPeak: 234480 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Aug 28 02:10:12 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: 2461229.75814948 08.07.2026 06:11:34.115 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
First image: 2461229.75814948 08.07.2026 06:11:34.115 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Last image: 2461280.64746398 28.08.2026 03:32:10.888 /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 71
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.16
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: 82 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 103261
Objects passed selection criteria: 103077
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 73400
Average stars matched: 68074.8 (92.7449 %)
Memory usage VmPeak: 565844 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Aug 28 02:12:52 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
SExtractor catalog cache: saved Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.cat to cache
SExtractor catalog cache: saved Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.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/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.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: 2461280.64692631
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_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits exists and is non-empty
wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits exists and is non-empty
wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits exists and is non-empty
wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits (1st reference image)
verification OK: wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Image size: 937.3'x625.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:46:55.925 -34:00:01.60 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_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits (1st new image)
verification OK: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
Image size: 936.8'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:46:58.501 -34:00:24.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:46:55.925 -34:00:01.60
Second-epoch image center 18:46:58.501 -34:00:24.34
Angular distance between the image centers 0.0109 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits (2nd new image)
verification OK: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Image size: 936.8'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:46:56.184 -34:00:26.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:46:55.925 -34:00:01.60
Second-epoch image center 18:46:56.184 -34:00:26.41
Angular distance between the image centers 0.0069 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 18:46:58.501 -34:00:24.34
Second-epoch second image center 18:46:56.184 -34:00:26.41
Angular distance between the image centers 0.00802 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits &> /tmp/tmp.UDb2IqtRKY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits &> /tmp/tmp.ggClP9MACv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits &> /tmp/tmp.Jq2l18FTcr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits &> /tmp/tmp.xsNTA8M5mP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.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_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits and wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits and wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat
Found non-empty wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits and wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat
The reference image (wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits) and catalog (wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat) found
'wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat' -> 'wcsmag.cat'
Read 9747 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.7337 to 291.6151 deg, Dec -39.2711 to -28.4566 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 271.7337 to 291.6151 deg, Dec -39.2711 to -28.4566 deg
Loaded 18854 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): 7751 out of 8000 total matches.
Matched with Tycho-2 8000 out of 9747 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.309400
a=0.000000 b=1.000000 c=22.309400
From vast_summary.log: estimated ref. image limiting mag.: -8.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.84
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9747 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.7337 to 291.6151 deg, Dec -39.2711 to -28.4566 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 271.7337 to 291.6151 deg, Dec -39.2711 to -28.4566 deg
Loaded 18854 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): 7751 out of 8000 total matches.
Matched with Tycho-2 8000 out of 9747 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Forced-photometry filter: calibrated wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits -> calib.txt_param_ref_wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits (aperture=6.0)
Read 9637 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.7334 to 291.6528 deg, Dec -39.2762 to -28.4569 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 271.7334 to 291.6528 deg, Dec -39.2762 to -28.4569 deg
Loaded 18877 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): 7647 out of 7892 total matches.
Matched with Tycho-2 7892 out of 9637 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
Forced-photometry filter: calibrated wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits -> calib.txt_param_ref_wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
2.3 pix Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
2.6 pix fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
2.6 pix fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Limiting magnitude estimates:
13.8 mag. Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
13.8 mag. Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
12.8 mag. fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
12.9 mag. fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.UDb2IqtRKY (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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits' -> 'wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
WCS-calibrated image found: wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Checking if the catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat corresponding to the image wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat corresponding to the image wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
WCS catalog name: wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=676, bad_region=1425, passed=9747
Got 9747 stars (including 7720 good ones) from the SExtractor catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat
util/solve_plate_with_UCAC5 got 9747 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 4818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 8601 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 8601 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 8601 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 4814 stars left (next iteration limit 5299)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits N_match=4814 sigma_overall_arcsec=0.668 sigma_q1_arcsec=0.630 sigma_q2_arcsec=0.611 sigma_q3_arcsec=0.750 sigma_q4_arcsec=0.600 n_q1=1680 n_q2=647 n_q3=1784 n_q4=703 worst_quadrant_to_overall_ratio=1.123
The image catalog is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits -region wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ggClP9MACv (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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits' -> 'wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
WCS-calibrated image found: wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
Checking if the catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat corresponding to the image wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat corresponding to the image wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
WCS catalog name: wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=703, bad_region=1428, passed=9637
Got 9637 stars (including 7580 good ones) from the SExtractor catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat
util/solve_plate_with_UCAC5 got 9637 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 4812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 8494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 8494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 8494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 4813 stars left (next iteration limit 5292)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits N_match=4813 sigma_overall_arcsec=0.660 sigma_q1_arcsec=0.627 sigma_q2_arcsec=0.606 sigma_q3_arcsec=0.745 sigma_q4_arcsec=0.579 n_q1=1671 n_q2=649 n_q3=1782 n_q4=711 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits -region wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Jq2l18FTcr (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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
WCS-calibrated image found: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
Checking if the catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat corresponding to the image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat corresponding to the image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
WCS catalog name: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=229, bad_region=1244, passed=4114
Got 4114 stars (including 2721 good ones) from the SExtractor catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat
util/solve_plate_with_UCAC5 got 4114 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 2682 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2616 matched stars entering correct_measured_positions(), 2616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2616 matched stars entering correct_measured_positions(), 3104 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 2683 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2617 matched stars entering correct_measured_positions(), 3104 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 2617 matched stars entering correct_measured_positions(), 3104 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 2617 stars left (next iteration limit 2877)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2617 robust_rms=5.973 arcsec worst_quadrant_rms=6.394 arcsec
SIP_REFIT: SIP order 3 trial: matched=2617 robust_rms=0.604 arcsec worst_quadrant_rms=0.681 arcsec
SIP_REFIT: SIP order 5 trial: matched=2617 robust_rms=0.570 arcsec worst_quadrant_rms=0.662 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=2617 robust_rms_before=0.877 arcsec robust_rms_before_corrected=0.710 arcsec robust_rms_after=0.604 arcsec worst_quadrant_rms_before=0.861 worst_quadrant_rms_after=0.681
verification OK: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
verification OK: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
Image size: 936.8'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:46:58.514 -34:00:24.79 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 4114 stars ###
'wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/correct_sextractor_wcs_catalog_usingxy2sky2117573.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 0.877 -> 0.604 arcsec)
WCS_QUALITY_DIAG: file=fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits N_match=2617 sigma_overall_arcsec=0.634 sigma_q1_arcsec=0.564 sigma_q2_arcsec=0.728 sigma_q3_arcsec=0.600 sigma_q4_arcsec=0.661 n_q1=784 n_q2=688 n_q3=627 n_q4=518 worst_quadrant_to_overall_ratio=1.148
The image catalog is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits -region wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.xsNTA8M5mP (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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
WCS-calibrated image found: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Checking if the catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat corresponding to the image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat corresponding to the image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
WCS catalog name: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=235, bad_region=1265, passed=4232
Got 4232 stars (including 2800 good ones) from the SExtractor catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat
util/solve_plate_with_UCAC5 got 4232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 2762 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2692 matched stars entering correct_measured_positions(), 2693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2692 matched stars entering correct_measured_positions(), 3214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 2763 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2692 matched stars entering correct_measured_positions(), 3214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 2692 matched stars entering correct_measured_positions(), 3214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 2692 stars left (next iteration limit 2961)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2692 robust_rms=6.067 arcsec worst_quadrant_rms=6.673 arcsec
SIP_REFIT: SIP order 3 trial: matched=2692 robust_rms=0.613 arcsec worst_quadrant_rms=0.690 arcsec
SIP_REFIT: SIP order 5 trial: matched=2692 robust_rms=0.586 arcsec worst_quadrant_rms=0.675 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=2692 robust_rms_before=0.867 arcsec robust_rms_before_corrected=0.708 arcsec robust_rms_after=0.613 arcsec worst_quadrant_rms_before=0.846 worst_quadrant_rms_after=0.690
verification OK: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
verification OK: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Image size: 936.8'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:46:56.187 -34:00:26.86 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 4232 stars ###
'wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/correct_sextractor_wcs_catalog_usingxy2sky2117658.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 0.867 -> 0.613 arcsec)
WCS_QUALITY_DIAG: file=fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits N_match=2692 sigma_overall_arcsec=0.636 sigma_q1_arcsec=0.532 sigma_q2_arcsec=0.752 sigma_q3_arcsec=0.591 sigma_q4_arcsec=0.690 n_q1=762 n_q2=748 n_q3=639 n_q4=543 worst_quadrant_to_overall_ratio=1.182
The image catalog is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits -region wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits to local_wcs_cache/
'wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits' -> 'local_wcs_cache/wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits'
Saving the final (post-refit) wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits to local_wcs_cache/
'wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits'
Saving the final (post-refit) wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits to local_wcs_cache/
'wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits' -> 'local_wcs_cache/wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits'
Saving the final (post-refit) wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits to local_wcs_cache/
'wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits' -> 'local_wcs_cache/wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits sigma_overall=0.668 worst_q_ratio=1.123
ref2=Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits sigma_overall=0.660 worst_q_ratio=1.128
new1=fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits sigma_overall=0.634 worst_q_ratio=1.148
new2=fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits sigma_overall=0.636 worst_q_ratio=1.182
reference average sigma_overall=0.664 worst_q_ratio=1.1255
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050_astrometric_residuals.png (4814 matched stars from wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.63 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051_astrometric_residuals.png (4813 matched stars from wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.64 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002_astrometric_residuals.png (2617 matched stars from wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003_astrometric_residuals.png (2692 matched stars from wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits'
Saving fully-calibrated image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits'
Preparing the HTML report for the field Sgr-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20513_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 20513_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 19:07:28.96 -36:22:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20774_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 20774_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:30:57.52 -31:08:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20920_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 20920_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:32:32.28 -34:58:39.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01938_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 01938_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:39:41.09 -36:48:41.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Sgr-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
SExtractor catalog cache: saved Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.cat to cache
SExtractor catalog cache: saved Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Creating symlink local_wcs_cache/wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits exists and is non-empty
wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits exists and is non-empty
wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits exists and is non-empty
wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits (1st reference image)
verification OK: wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Image size: 937.3'x625.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:46:55.925 -34:00:01.60 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_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits (1st new image)
verification OK: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
Image size: 936.8'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:46:58.514 -34:00:24.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:46:55.925 -34:00:01.60
Second-epoch image center 18:46:58.514 -34:00:24.79
Angular distance between the image centers 0.0110 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits (2nd new image)
verification OK: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Image size: 936.8'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 18:46:56.187 -34:00:26.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:46:55.925 -34:00:01.60
Second-epoch image center 18:46:56.187 -34:00:26.86
Angular distance between the image centers 0.0071 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 18:46:58.514 -34:00:24.79
Second-epoch second image center 18:46:56.187 -34:00:26.86
Angular distance between the image centers 0.00806 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits &> /tmp/tmp.qgjMETsiCZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits &> /tmp/tmp.VDTGVjYIPA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits &> /tmp/tmp.VsDXu7Jvy8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits &> /tmp/tmp.epg6n8Llfw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.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_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits and wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits and wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat
Found non-empty wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits and wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat
The reference image (wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits) and catalog (wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat) found
'wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat' -> 'wcsmag.cat'
Read 119127 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.6982 to 291.7315 deg, Dec -39.2735 to -28.4566 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 271.6982 to 291.7315 deg, Dec -39.2735 to -28.4566 deg
Loaded 18960 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): 14049 out of 15978 total matches.
Matched with Tycho-2 15978 out of 119127 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.071400
a=0.000000 b=1.000000 c=22.071400
From vast_summary.log: estimated ref. image limiting mag.: -8.16
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.91
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.91
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 119127 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.6982 to 291.7315 deg, Dec -39.2735 to -28.4566 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 271.6982 to 291.7315 deg, Dec -39.2735 to -28.4566 deg
Loaded 18960 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): 14049 out of 15978 total matches.
Matched with Tycho-2 15978 out of 119127 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Forced-photometry filter: calibrated wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits -> calib.txt_param_ref_wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits (aperture=4.4)
Read 123059 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.6989 to 291.7304 deg, Dec -39.2762 to -28.4568 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 271.6989 to 291.7304 deg, Dec -39.2762 to -28.4568 deg
Loaded 18963 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): 14010 out of 15963 total matches.
Matched with Tycho-2 15963 out of 123059 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
Forced-photometry filter: calibrated wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits -> calib.txt_param_ref_wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 56 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
2.1 pix Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
2.4 pix fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
2.4 pix fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Limiting magnitude estimates:
13.9 mag. Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
13.9 mag. Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
13.0 mag. fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
13.1 mag. fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.qgjMETsiCZ (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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits' -> 'wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
WCS-calibrated image found: wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
Checking if the catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat corresponding to the image wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat corresponding to the image wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits
WCS catalog name: wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=8489, bad_region=10831, passed=119125
Got 119125 stars (including 100241 good ones) from the SExtractor catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat
util/solve_plate_with_UCAC5 got 119125 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 4834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 111087 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 111087 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 111086 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 4830 stars left (next iteration limit 5315)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits N_match=4830 sigma_overall_arcsec=0.667 sigma_q1_arcsec=0.627 sigma_q2_arcsec=0.611 sigma_q3_arcsec=0.743 sigma_q4_arcsec=0.632 n_q1=1709 n_q2=665 n_q3=1727 n_q4=729 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits -region wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.VDTGVjYIPA (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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits' -> 'wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
WCS-calibrated image found: wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
Checking if the catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat corresponding to the image wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat corresponding to the image wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits
WCS catalog name: wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=8929, bad_region=11024, passed=123053
Got 123053 stars (including 103547 good ones) from the SExtractor catalog wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat
util/solve_plate_with_UCAC5 got 123053 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 4828 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 114882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4826 matched stars entering correct_measured_positions(), 114882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 4826 matched stars entering correct_measured_positions(), 114882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 4826 stars left (next iteration limit 5307)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits N_match=4826 sigma_overall_arcsec=0.630 sigma_q1_arcsec=0.601 sigma_q2_arcsec=0.598 sigma_q3_arcsec=0.710 sigma_q4_arcsec=0.595 n_q1=1716 n_q2=667 n_q3=1722 n_q4=721 worst_quadrant_to_overall_ratio=1.127
The image catalog is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits -region wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.VsDXu7Jvy8 (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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
WCS-calibrated image found: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
Checking if the catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat corresponding to the image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat corresponding to the image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
WCS catalog name: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2440, bad_region=11753, passed=48062
Got 48062 stars (including 35065 good ones) from the SExtractor catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat
util/solve_plate_with_UCAC5 got 48062 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 4815 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 39049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 39049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 39048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 4812 stars left (next iteration limit 5295)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4812 robust_rms=6.029 arcsec worst_quadrant_rms=6.834 arcsec
SIP_REFIT: SIP order 3 trial: matched=4812 robust_rms=0.612 arcsec worst_quadrant_rms=0.689 arcsec
SIP_REFIT: SIP order 5 trial: matched=4812 robust_rms=0.582 arcsec worst_quadrant_rms=0.663 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4812 robust_rms_before=0.613 arcsec robust_rms_before_corrected=0.670 arcsec robust_rms_after=0.612 arcsec worst_quadrant_rms_before=0.691 worst_quadrant_rms_after=0.689
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.691 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits N_match=4812 sigma_overall_arcsec=0.656 sigma_q1_arcsec=0.556 sigma_q2_arcsec=0.816 sigma_q3_arcsec=0.538 sigma_q4_arcsec=0.657 n_q1=1553 n_q2=1187 n_q3=1207 n_q4=865 worst_quadrant_to_overall_ratio=1.244
The image catalog is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits -region wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.epg6n8Llfw (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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
WCS-calibrated image found: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Checking if the catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat corresponding to the image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat corresponding to the image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
WCS catalog name: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2775, bad_region=12096, passed=51147
Got 51147 stars (including 37611 good ones) from the SExtractor catalog wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat
util/solve_plate_with_UCAC5 got 51147 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 4818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 41964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 41964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 41964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 4814 stars left (next iteration limit 5298)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4814 robust_rms=5.962 arcsec worst_quadrant_rms=6.630 arcsec
SIP_REFIT: SIP order 3 trial: matched=4814 robust_rms=0.595 arcsec worst_quadrant_rms=0.678 arcsec
SIP_REFIT: SIP order 5 trial: matched=4814 robust_rms=0.577 arcsec worst_quadrant_rms=0.677 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4814 robust_rms_before=0.598 arcsec robust_rms_before_corrected=0.667 arcsec robust_rms_after=0.595 arcsec worst_quadrant_rms_before=0.670 worst_quadrant_rms_after=0.678
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.670 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits N_match=4814 sigma_overall_arcsec=0.650 sigma_q1_arcsec=0.554 sigma_q2_arcsec=0.795 sigma_q3_arcsec=0.539 sigma_q4_arcsec=0.714 n_q1=1517 n_q2=1232 n_q3=1200 n_q4=865 worst_quadrant_to_overall_ratio=1.224
The image catalog is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits -region wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-31-24_20.00sec_-0.00C_LIGHT_0002.fits
Saving fully-calibrated image wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.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_2026-08-27_CI_Sgr-06-Q2b1x1_225736_TTUQ2b1x1_2861028_dlxQbrCi/wcs_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003.fits
Preparing the HTML report for the field Sgr-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:48:54.05 -30:59:27.6: 11.91 +/- 0.03 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:35:44.64 -34:02:11.9: 11.98 +/- 0.03 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 19:05:15.73 -32:38:18.2: 12.29 +/- 0.04 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:37:40.50 -33:32:42.2: 11.43 +/- 0.02 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 19:01:53.46 -36:20:09.0: 11.99 +/- 0.03 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:26:42.74 -32:22:03.5: 11.59 +/- 0.03 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 19:02:49.74 -31:21:10.7: 12.15 +/- 0.04 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:36:40.81 -29:50:51.5: 10.80 +/- 0.01 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 19:01:53.46 -36:20:09.0: 11.90 +/- 0.03 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:35:44.64 -34:02:11.9: 12.02 +/- 0.03 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 19:05:15.73 -32:38:18.2: 12.25 +/- 0.04 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 19:02:49.74 -31:21:10.7: 12.12 +/- 0.03 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:48:54.05 -30:59:27.6: 11.93 +/- 0.03 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:26:42.74 -32:22:03.5: 11.58 +/- 0.03 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:37:40.50 -33:32:42.2: 11.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.02
Forced photometry reference-image weighted average: 12.00 +/- 0.02
Forced photometry reference-image weighted average: 12.26 +/- 0.03
Forced photometry filter REJECTED candidate at 19:01:53.46 -36:20:09.0: ref_mag=11.94 +/- 0.02 new_mean_mag=11.8786 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.13 +/- 0.03
Forced photometry reference-image weighted average: 11.92 +/- 0.02
Forced photometry filter REJECTED candidate at 18:35:44.64 -34:02:11.9: ref_mag=12.00 +/- 0.02 new_mean_mag=11.8860 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:05:15.73 -32:38:18.2: ref_mag=12.26 +/- 0.03 new_mean_mag=12.3641 delta=-0.10 (need > 0.90)
Forced photometry reference-image weighted average: 11.58 +/- 0.02
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Forced photometry filter REJECTED candidate at 19:02:49.74 -31:21:10.7: ref_mag=12.13 +/- 0.03 new_mean_mag=12.2935 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:48:54.05 -30:59:27.6: ref_mag=11.92 +/- 0.02 new_mean_mag=12.3485 delta=-0.43 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:26:42.74 -32:22:03.5: ref_mag=11.58 +/- 0.02 new_mean_mag=11.5135 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:37:40.50 -33:32:42.2: ref_mag=11.44 +/- 0.01 new_mean_mag=11.4682 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:36:40.81 -29:50:51.5: 10.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.01
Forced photometry filter REJECTED candidate at 18:36:40.81 -29:50:51.5: ref_mag=10.78 +/- 0.01 new_mean_mag=10.4652 delta=0.31 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 19:06:15.28 -34:46:01.4: 12.01 +/- 0.03 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:30:48.59 -31:28:26.0: 12.15 +/- 0.04 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:46:44.44 -31:43:54.7: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 19:09:02.05 -36:52:12.2: 12.48 +/- 0.06 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:45:13.79 -35:52:16.0: 12.25 +/- 0.05 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:35:26.97 -32:54:28.2: 12.62 +/- 0.07 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:48:45.61 -30:05:20.2: 12.52 +/- 0.06 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:29:04.31 -29:54:07.6: 12.38 +/- 0.06 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 19:06:15.28 -34:46:01.4: 12.09 +/- 0.04 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:30:48.59 -31:28:26.0: 12.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.02
Forced photometry filter REJECTED candidate at 19:06:15.28 -34:46:01.4: ref_mag=12.05 +/- 0.02 new_mean_mag=11.8714 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 12.15 +/- 0.03
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:46:44.44 -31:43:54.7: 14.65 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 18:30:48.59 -31:28:26.0: ref_mag=12.15 +/- 0.03 new_mean_mag=11.9821 delta=0.17 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 19:09:02.05 -36:52:12.2: 12.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.04
Forced photometry filter REJECTED candidate at 19:09:02.05 -36:52:12.2: ref_mag=12.42 +/- 0.04 new_mean_mag=12.0411 delta=0.38 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:45:13.79 -35:52:16.0: 12.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.03
Forced photometry filter REJECTED candidate at 18:45:13.79 -35:52:16.0: ref_mag=12.17 +/- 0.03 new_mean_mag=12.0280 delta=0.15 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:48:45.61 -30:05:20.2: 12.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.04
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:29:04.31 -29:54:07.6: 12.24 +/- 0.05 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:35:26.97 -32:54:28.2: 12.62 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 18:48:45.61 -30:05:20.2: ref_mag=12.49 +/- 0.04 new_mean_mag=12.4596 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 12.62 +/- 0.05
Forced photometry reference-image weighted average: 12.29 +/- 0.04
Forced photometry filter REJECTED candidate at 18:35:26.97 -32:54:28.2: ref_mag=12.62 +/- 0.05 new_mean_mag=12.1773 delta=0.44 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:29:04.31 -29:54:07.6: ref_mag=12.29 +/- 0.04 new_mean_mag=12.2144 delta=0.08 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:52:11.45 -32:49:44.5: 14.62 +/- 0.35 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:52:11.45 -32:49:44.5: 14.31 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.21
Forced photometry filter KEPT candidate at 18:52:11.45 -32:49:44.5: ref_mag=14.42 +/- 0.21 new_mean_mag=12.5406 delta=1.88 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:26:49.04 -34:48:44.2: 13.16 +/- 0.11 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 19:05:22.34 -34:49:32.3: 13.94 +/- 0.20 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:33:04.17 -30:39:07.2: 12.48 +/- 0.05 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:26:49.04 -34:48:44.2: 13.29 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.08
Forced photometry filter KEPT candidate at 18:26:49.04 -34:48:44.2: ref_mag=13.21 +/- 0.08 new_mean_mag=12.0605 delta=1.15 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 19:05:22.34 -34:49:32.3: 14.60 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.94 +/- 0.20
Forced photometry filter KEPT candidate at 19:05:22.34 -34:49:32.3: ref_mag=13.94 +/- 0.20 new_mean_mag=12.1158 delta=1.82 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:33:04.17 -30:39:07.2: 12.44 +/- 0.05 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:28:46.70 -30:04:38.2: 13.32 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.04
Forced photometry filter KEPT candidate at 18:33:04.17 -30:39:07.2: ref_mag=12.46 +/- 0.04 new_mean_mag=11.3431 delta=1.12 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:28:46.70 -30:04:38.2: 13.38 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.09
Forced photometry filter KEPT candidate at 18:28:46.70 -30:04:38.2: ref_mag=13.35 +/- 0.09 new_mean_mag=12.0930 delta=1.26 (need > 0.90)
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-11-34_20.00sec_5.00C_LIGHT_0050.fits at 18:28:26.87 -33:48:15.9: 11.31 +/- 0.02 detection
Forced photometry on wcs_Sgr-06-Q2b1x1_2026-07-08_01-12-13_20.00sec_4.90C_LIGHT_0051.fits at 18:28:26.87 -33:48:15.9: 11.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.02
Forced photometry filter KEPT candidate at 18:28:26.87 -33:48:15.9: ref_mag=11.30 +/- 0.02 new_mean_mag=10.3400 delta=0.96 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out149214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out102541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48776.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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: 5s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143144_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143144_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143145_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143145_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143148_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143148_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143150_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143150_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:54:03.67 -36:39:22.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143151_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143151_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143152_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143152_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143155_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143155_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143156_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143156_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143157_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143157_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 19:01:32.38 -31:13:41.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143158_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143158_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 19:07:28.96 -36:22:26.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143839_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 143839_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144004_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 144004_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:48:49.52 -36:41:59.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144088_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 144088_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144579_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 144579_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:36:14.40 -35:28:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144812_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 144812_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:36:48.36 -36:02:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144836_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 144836_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
Rejecting candidate due to large distance (28.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144964_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 144964_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:58:31.62 -35:03:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145125_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 145125_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:31:49.55 -33:37:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145135_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 145135_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:33:41.67 -30:09:27.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145607_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 145607_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:29:18.16 -34:54:06.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145956_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 145956_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:32:00.38 -31:11:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146103_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 146103_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146718_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 146718_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:43:48.18 -31:48:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146882_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 146882_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146884_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 146884_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:31:08.11 -29:50:38.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146920_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
Preparing report for the candidate 146920_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146933_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 146933_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146952_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 146952_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147192_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 147192_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:33:16.66 -34:12:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147209_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 147209_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147218_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 147218_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147849_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 147849_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147911_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 147911_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:38:45.76 -34:33:27.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148156_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 148156_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:27:47.93 -31:21:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148354_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 148354_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:51:29.40 -36:27:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148462_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 148462_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:36:46.40 -34:40:14.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149214_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 149214_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:52:11.45 -32:49:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.007 6735921596883429888 283.04774598151 -32.82874981407 12.1879 10.2656 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149313_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 149313_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:42:13.39 -29:47:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149371_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 149371_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:44:01.27 -30:01:42.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21822_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 21822_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:24:52.55 -36:11:00.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36822_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
Preparing report for the candidate 36822_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141269_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 141269_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:40:27.32 -33:13:34.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23570_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 23570_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:53:29.82 -36:07:28.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37049_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
Preparing report for the candidate 37049_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15057_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 15057_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:41:15.25 -37:02:33.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66880_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 66880_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:38:21.21 -32:35:52.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106946_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
Preparing report for the candidate 106946_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133494_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 133494_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:37:41.42 -30:48:13.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102541_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
Preparing report for the candidate 102541_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86460_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 86460_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:49:31.32 -31:10:06.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37395_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 37395_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:43:35.48 -34:52:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35550_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 35550_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:32:32.28 -34:58:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89654_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 89654_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:47:06.43 -31:46:47.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110583_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 110583_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks
**** FOUND 18:30:57.53 -31:08:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48776_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
Preparing report for the candidate 48776_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16719_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003
The candidate 16719_fd_Sgr-06-Q2b1x1_2026-08-27_22-32-10_20.00sec_-0.00C_LIGHT_0003 did not pass the final checks