This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 25.1851 2461185.6851 11.60 16:34:03.03 -22:32:44.2
355.72974 16.79356 galactic Oph Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.24 Themis 2 0 2 11.7 -0 0
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 16:34:03.03 -22:32:44.2: 15.14 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 16:34:03.03 -22:32:44.2: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461185.6851,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260525.1851 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.1851 2461185.6851 12.27 16:28:45.43 -25:06:08.2
352.88382 16.05193 galactic Sco Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.674 Rachele 3 0 3 12.2 -0 -0
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 16:28:45.43 -25:06:08.2: 15.12 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 16:28:45.43 -25:06:08.2: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461185.6851,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260525.1851 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.1851 2461185.6851 12.94 16:17:05.97 -26:53:47.3
349.66278 16.78238 galactic Sco Second-epoch detections are separated by 1.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.556 Phyllis 3 0 3 13.0 0 -0
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 16:17:05.97 -26:53:47.3: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 16:17:05.97 -26:53:47.3: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461185.6851,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260525.1851 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.1851 2461185.6851 13.14 16:17:42.49 -27:08:00.3
349.58017 16.52112 galactic Sco Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.254 Augusta 4 -0 4 13.5 -0 -0
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 16:17:42.49 -27:08:00.3: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 16:17:42.49 -27:08:00.3: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461185.6851,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260525.1851 13.14CV 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: 2461139.81765986 09.04.2026 07:37:15.812 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
First image: 2461139.81765986 09.04.2026 07:37:15.812 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
Last image: 2461185.68544284 25.05.2026 04:26:52.261 /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.38
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4009
Objects passed selection criteria: 4008
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 3495.5
Average stars matched: 3442.5 (98.4838 %)
Memory usage VmPeak: 110800 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 24 23:36:21 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: 2461139.81765986 09.04.2026 07:37:15.812 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
First image: 2461139.81765986 09.04.2026 07:37:15.812 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
Last image: 2461185.68544284 25.05.2026 04:26:52.261 /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 44
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.99
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: 17 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 41508
Objects passed selection criteria: 41448
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 37004.5
Average stars matched: 36261.5 (97.9921 %)
Memory usage VmPeak: 150360 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 24 23:39:06 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.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/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461185.68484926
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_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits'
wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits'
wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits'
wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits (1st reference image)
verification OK: wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
Image size: 941.9'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:12.320 -25:59:25.30 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
Image size: 937.8'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:19:09.950 -25:59:37.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:12.320 -25:59:25.30
Second-epoch image center 16:19:09.950 -25:59:37.86
Angular distance between the image centers 0.0095 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
Image size: 937.8'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:19:12.680 -25:59:49.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:12.320 -25:59:25.30
Second-epoch image center 16:19:12.680 -25:59:49.48
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 16:19:09.950 -25:59:37.86
Second-epoch second image center 16:19:12.680 -25:59:49.48
Angular distance between the image centers 0.01072 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits &> /tmp/tmp.eBbmDDwbet
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits &> /tmp/tmp.akO9EbOhAt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits &> /tmp/tmp.OHvVI0UEpM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits &> /tmp/tmp.aeJcLhmjQA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.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_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits and wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits and wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat
Found non-empty wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits and wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat
The reference image (wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits) and catalog (wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat) found
'wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat' -> 'wcsmag.cat'
Read 6377 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3884 to 253.5840 deg, Dec -31.5113 to -20.0797 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 235.3884 to 253.5840 deg, Dec -31.5113 to -20.0797 deg
Loaded 8583 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): 4654 out of 4825 total matches.
Matched with Tycho-2 4825 out of 6377 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.627400
a=0.000000 b=1.000000 c=22.627400
From vast_summary.log: estimated ref. image limiting mag.: -8.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6377 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3884 to 253.5840 deg, Dec -31.5113 to -20.0797 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 235.3884 to 253.5840 deg, Dec -31.5113 to -20.0797 deg
Loaded 8583 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): 4654 out of 4825 total matches.
Matched with Tycho-2 4825 out of 6377 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits:
Forced-photometry filter: calibrated wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits -> calib.txt_param_ref_wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits (aperture=6.1)
Read 5296 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.4154 to 253.5845 deg, Dec -31.5353 to -20.0794 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 235.4154 to 253.5845 deg, Dec -31.5353 to -20.0794 deg
Loaded 8596 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): 4065 out of 4156 total matches.
Matched with Tycho-2 4156 out of 5296 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits:
Forced-photometry filter: calibrated wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits -> calib.txt_param_ref_wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
2.2 pix Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
2.5 pix fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
2.5 pix fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
2.1 pix wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
2.2 pix wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
Limiting magnitude estimates:
14.2 mag. Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
14.0 mag. Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
13.4 mag. fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
13.4 mag. fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.eBbmDDwbet (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits' -> 'wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=576, passed=6377
Got 6377 stars (including 5785 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat
util/solve_plate_with_UCAC5 got 6377 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 6230 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 6232 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 6231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits N_match=961 sigma_overall_arcsec=0.403 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.435 sigma_q3_arcsec=0.424 sigma_q4_arcsec=0.528 n_q1=284 n_q2=266 n_q3=255 n_q4=156 worst_quadrant_to_overall_ratio=1.310
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits -region wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.akO9EbOhAt (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits' -> 'wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=393, passed=5296
Got 5296 stars (including 4896 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat
util/solve_plate_with_UCAC5 got 5296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5187 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5186 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits N_match=963 sigma_overall_arcsec=0.338 sigma_q1_arcsec=0.267 sigma_q2_arcsec=0.422 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.435 n_q1=284 n_q2=244 n_q3=276 n_q4=159 worst_quadrant_to_overall_ratio=1.289
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits -region wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OHvVI0UEpM (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=300, passed=3653
Got 3653 stars (including 3350 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat
util/solve_plate_with_UCAC5 got 3653 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 3577 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
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 3574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 3571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 954 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits N_match=954 sigma_overall_arcsec=0.698 sigma_q1_arcsec=0.491 sigma_q2_arcsec=1.329 sigma_q3_arcsec=0.496 sigma_q4_arcsec=1.137 n_q1=291 n_q2=263 n_q3=232 n_q4=168 worst_quadrant_to_overall_ratio=1.905
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits -region wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.aeJcLhmjQA (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=292, passed=3692
Got 3692 stars (including 3392 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 3692 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 3606 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
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 3606 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 3606 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits N_match=957 sigma_overall_arcsec=0.688 sigma_q1_arcsec=0.487 sigma_q2_arcsec=1.207 sigma_q3_arcsec=0.512 sigma_q4_arcsec=1.157 n_q1=289 n_q2=260 n_q3=239 n_q4=169 worst_quadrant_to_overall_ratio=1.754
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits -region wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits sigma_overall=0.403 worst_q_ratio=1.310
ref2=Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits sigma_overall=0.338 worst_q_ratio=1.289
new1=fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits sigma_overall=0.698 worst_q_ratio=1.905
new2=fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits sigma_overall=0.688 worst_q_ratio=1.754
reference average sigma_overall=0.3705 worst_q_ratio=1.2995
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190_astrometric_residuals.png (961 matched stars from wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174_astrometric_residuals.png (963 matched stars from wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106_astrometric_residuals.png (954 matched stars from wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107_astrometric_residuals.png (957 matched stars from wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits'
Preparing the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 16:23:31.73 -26:33:04.5: 11.31 +/- 0.05 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 16:23:31.73 -26:33:04.5: 11.32 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.31 +/- 0.04
Forced photometry filter REJECTED candidate at 16:23:31.73 -26:33:04.5: ref_mag=11.31 +/- 0.04 new_mean_mag=10.8375 delta=0.47 (need > 0.90)
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20124_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 20124_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:17:39.23 -22:56:40.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20146_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 20146_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:10:46.59 -23:03:57.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20154_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 20154_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:02:42.68 -26:54:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20165_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 20165_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20171_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 20171_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:09:51.66 -25:08:41.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04777_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 04777_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:04:36.15 -24:06:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02298_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 02298_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:38:12.94 -28:34:09.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20020_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 20020_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:17:40.35 -22:53:35.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits exists and is non-empty
wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits exists and is non-empty
wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits exists and is non-empty
wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits (1st reference image)
verification OK: wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
Image size: 941.9'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:12.320 -25:59:25.30 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
Image size: 937.8'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:19:09.950 -25:59:37.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:12.320 -25:59:25.30
Second-epoch image center 16:19:09.950 -25:59:37.86
Angular distance between the image centers 0.0095 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
Image size: 937.8'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:19:12.680 -25:59:49.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:12.320 -25:59:25.30
Second-epoch image center 16:19:12.680 -25:59:49.48
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 16:19:09.950 -25:59:37.86
Second-epoch second image center 16:19:12.680 -25:59:49.48
Angular distance between the image centers 0.01072 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits &> /tmp/tmp.f2Q9U2eWO0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits &> /tmp/tmp.ql7cLO32ei
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits &> /tmp/tmp.tIPBhdzGSC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits &> /tmp/tmp.eZWd57a3i5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.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_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits and wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits and wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat
Found non-empty wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits and wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat
The reference image (wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits) and catalog (wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat) found
'wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat' -> 'wcsmag.cat'
Read 70432 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3318 to 253.5851 deg, Dec -31.5213 to -20.0064 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 235.3318 to 253.5851 deg, Dec -31.5213 to -20.0064 deg
Loaded 8671 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): 6325 out of 7000 total matches.
Matched with Tycho-2 7000 out of 70432 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.413100
a=0.000000 b=1.000000 c=22.413100
From vast_summary.log: estimated ref. image limiting mag.: -7.99
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 70432 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3318 to 253.5851 deg, Dec -31.5213 to -20.0064 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 235.3318 to 253.5851 deg, Dec -31.5213 to -20.0064 deg
Loaded 8671 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): 6325 out of 7000 total matches.
Matched with Tycho-2 7000 out of 70432 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits:
Forced-photometry filter: calibrated wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits -> calib.txt_param_ref_wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits (aperture=4.3)
Read 56523 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3388 to 253.5858 deg, Dec -31.5513 to -20.0429 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 235.3388 to 253.5858 deg, Dec -31.5513 to -20.0429 deg
Loaded 8686 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): 6533 out of 7007 total matches.
Matched with Tycho-2 7007 out of 56523 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits:
Forced-photometry filter: calibrated wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits -> calib.txt_param_ref_wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 33 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
2.1 pix Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
2.3 pix fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
2.3 pix fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
2.0 pix wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
2.1 pix wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
Limiting magnitude estimates:
14.4 mag. Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
14.2 mag. Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
13.7 mag. fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
13.7 mag. fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.f2Q9U2eWO0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits' -> 'wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=3556, passed=70421
Got 70421 stars (including 66735 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat
util/solve_plate_with_UCAC5 got 70421 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 68366 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 68366 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 68364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits N_match=968 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.422 sigma_q4_arcsec=0.480 n_q1=299 n_q2=278 n_q3=240 n_q4=151 worst_quadrant_to_overall_ratio=1.236
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits -region wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ql7cLO32ei (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits' -> 'wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2201, passed=56519
Got 56519 stars (including 54206 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat
util/solve_plate_with_UCAC5 got 56519 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.6 to -20.0)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 55146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.6 to -20.0)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 55149 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 55148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits N_match=967 sigma_overall_arcsec=0.323 sigma_q1_arcsec=0.263 sigma_q2_arcsec=0.394 sigma_q3_arcsec=0.309 sigma_q4_arcsec=0.371 n_q1=294 n_q2=251 n_q3=268 n_q4=154 worst_quadrant_to_overall_ratio=1.218
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits -region wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tIPBhdzGSC (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1411, passed=34684
Got 34684 stars (including 33233 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat
util/solve_plate_with_UCAC5 got 34684 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 33905 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
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 33904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 33903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits N_match=959 sigma_overall_arcsec=0.690 sigma_q1_arcsec=0.526 sigma_q2_arcsec=1.104 sigma_q3_arcsec=0.527 sigma_q4_arcsec=1.170 n_q1=312 n_q2=237 n_q3=247 n_q4=163 worst_quadrant_to_overall_ratio=1.696
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits -region wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eZWd57a3i5 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1383, passed=34824
Got 34824 stars (including 33397 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 34824 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 33959 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
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 33957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 33956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits N_match=961 sigma_overall_arcsec=0.677 sigma_q1_arcsec=0.508 sigma_q2_arcsec=1.119 sigma_q3_arcsec=0.533 sigma_q4_arcsec=1.228 n_q1=310 n_q2=242 n_q3=248 n_q4=161 worst_quadrant_to_overall_ratio=1.814
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits -region wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-00_20.00sec_5.00C_LIGHT_0106.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-24_CI_Sco-02-Q2b1x1_233404_TTUQ2b1x1_2055621_429HYrrM/wcs_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107.fits
Preparing the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 16:28:45.43 -25:06:08.2: 15.12 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 15:53:25.23 -27:41:38.8: 12.11 +/- 0.03 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 15:52:04.06 -22:17:36.0: 12.43 +/- 0.03 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 16:34:03.03 -22:32:44.2: 15.14 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 16:17:05.97 -26:53:47.3: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 16:28:45.43 -25:06:08.2: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 15:53:25.23 -27:41:38.8: 12.07 +/- 0.04 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 16:34:03.03 -22:32:44.2: 14.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.09 +/- 0.02
Forced photometry filter REJECTED candidate at 15:53:25.23 -27:41:38.8: ref_mag=12.09 +/- 0.02 new_mean_mag=12.1077 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 15:52:04.06 -22:17:36.0: 12.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.03
Forced photometry filter REJECTED candidate at 15:52:04.06 -22:17:36.0: ref_mag=12.43 +/- 0.03 new_mean_mag=12.7676 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-09_02-37-15_20.00sec_-5.00C_LIGHTs_0190.fits at 16:17:42.49 -27:08:00.3: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 16:17:05.97 -26:53:47.3: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-55-38_20.00sec_-4.90C_LIGHTs_0174.fits at 16:17:42.49 -27:08:00.3: 14.95 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out82496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83074.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 82327_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82327_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 82333_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82333_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
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Considering the candidate 82334_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82334_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:00:24.77 -23:27:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82339_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82339_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:09:46.76 -28:06:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82496_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
Preparing report for the candidate 82496_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
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Considering the candidate 82625_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82625_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:02:33.33 -26:10:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82642_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82642_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:11:03.45 -25:39:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82644_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82644_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
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Considering the candidate 82657_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
Preparing report for the candidate 82657_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
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Considering the candidate 82680_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82680_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:11:41.70 -27:03:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82776_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82776_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 15:55:38.34 -29:15:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82788_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82788_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:10:17.23 -30:14:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82795_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82795_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:07:52.16 -24:29:05.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82893_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 82893_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:37:25.75 -28:05:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82932_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
Preparing report for the candidate 82932_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
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Considering the candidate 83042_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 83042_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 83054_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 83054_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:29:28.72 -27:58:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83074_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
Preparing report for the candidate 83074_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
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Considering the candidate 83128_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 83128_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:32:18.20 -22:12:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83132_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 83132_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:31:43.24 -26:02:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35045_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 35045_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:03:53.83 -26:48:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41233_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 41233_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:23:31.91 -26:24:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56554_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 56554_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:17:40.35 -22:53:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69173_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 69173_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:15:22.07 -24:18:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24486_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 24486_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:38:12.95 -28:34:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81006_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 81006_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:05:30.91 -23:28:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81002_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 81002_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:37:31.73 -30:06:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57096_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 57096_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:17:39.22 -22:56:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29755_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 29755_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:38:50.53 -28:01:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59244_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 59244_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:10:46.59 -23:03:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33935_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 33935_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 16:02:42.69 -26:54:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67403_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 67403_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks
**** FOUND 15:59:23.87 -23:46:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69019_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107
The candidate 69019_fd_Sco-02-Q2b1x1_2026-05-24_23-26-52_20.00sec_4.90C_LIGHT_0107 did not pass the final checks