This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE
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 07 26.4086 2461247.9086 13.96 03:12:13.95 +15:39:32.9
165.74930 -35.25331 galactic Ari Second-epoch detections are separated by 4.0" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.62 Erato -1 -0 1 14.2 -0 0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:12:13.95 +15:39:32.9: 16.58 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:12:13.95 +15:39:32.9: 16.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.4086* 03 12 13.95 +15 39 32.9 14.0 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461247.9086,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260726.4086 13.96CV 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 07 26.4086 2461247.9086 13.73 03:59:34.20 +16:02:31.6
175.17618 -27.19146 galactic Tau Second-epoch detections are separated by 1.6" and 0.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.53 Kalypso -1 2 2 13.8 -0 0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:59:34.20 +16:02:31.6: 16.51 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:59:34.20 +16:02:31.6: 16.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.4086* 03 59 34.20 +16 02 31.6 13.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461247.9086,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260726.4086 13.73CV 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 07 26.4086 2461247.9086 14.01 03:54:50.77 +14:02:23.0
175.96018 -29.39002 galactic Tau Second-epoch detections are separated by 5.4" and 0.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:54:50.77 +14:02:23.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:54:50.77 +14:02:23.0: 16.62 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:54:50.77 +14:02:23.0: 16.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.4086* 03 54 50.77 +14 02 23.0 14.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.9086,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.4086 14.01CV 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 07 26.4086 2461247.9086 14.14 03:06:26.67 +17:56:08.2
162.71697 -34.30539 galactic Ari Second-epoch detections are separated by 3.6" and 0.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:06:26.67 +17:56:08.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:06:26.67 +17:56:08.2: 16.47 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:06:26.67 +17:56:08.2: 16.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.4086* 03 06 26.67 +17 56 08.2 14.1 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.9086,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.4086 14.14CV 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: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
First image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
Last image: 2461247.90879172 26.07.2026 09:48:29.605 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: unknown
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.07
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 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): 11076
Objects passed selection criteria: 11020
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 7751.5
Average stars matched: 7581.25 (97.8037 %)
Memory usage VmPeak: 236848 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 26 09:40:28 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: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
First image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
Last image: 2461247.90879172 26.07.2026 09:48:29.605 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 46
FILTER key from ref. img. header: unknown
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.81
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: 38 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): 56589
Objects passed selection criteria: 56435
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 41102.8
Average stars matched: 39833.5 (96.912 %)
Memory usage VmPeak: 277568 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 26 09:49:10 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.cat to cache
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.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/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.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: 2461247.90831432
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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits exists and is non-empty
Saving wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits to local_wcs_cache/
'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits' -> 'local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits'
wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits exists and is non-empty
Saving wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits to local_wcs_cache/
'wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits' -> 'local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits'
wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits exists and is non-empty
Saving wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits to local_wcs_cache/
'wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits' -> 'local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits'
wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits exists and is non-empty
Saving wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits to local_wcs_cache/
'wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits' -> 'local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits (1st reference image)
verification OK: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:20.346 +13:59:54.22 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_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits (1st new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
Image size: 941.7'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:19.652 +13:57:39.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:33:20.346 +13:59:54.22
Second-epoch image center 03:33:19.652 +13:57:39.49
Angular distance between the image centers 0.0375 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits (2nd new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
Image size: 941.7'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:19.875 +13:57:41.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:33:20.346 +13:59:54.22
Second-epoch image center 03:33:19.875 +13:57:41.78
Angular distance between the image centers 0.0368 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 03:33:19.652 +13:57:39.49
Second-epoch second image center 03:33:19.875 +13:57:41.78
Angular distance between the image centers 0.00110 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00110 deg. (min. required shift: 0.00164 deg.)
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits &> /tmp/tmp.6HRczu1L8M
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits &> /tmp/tmp.ZiGx6jp4vW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits &> /tmp/tmp.PHfh5o1sAk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits &> /tmp/tmp.mxInStmApi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat
The reference image (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits) and catalog (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat) found
'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat' -> 'wcsmag.cat'
Read 11518 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0644 to 61.6418 deg, Dec +8.6212 to +19.2874 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 45.0644 to 61.6418 deg, Dec 8.6212 to 19.2874 deg
Loaded 4359 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): 3495 out of 3755 total matches.
Matched with Tycho-2 3755 out of 11518 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.930100
a=0.000000 b=1.000000 c=22.930100
From vast_summary.log: estimated ref. image limiting mag.: -7.07
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.86
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11518 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0644 to 61.6418 deg, Dec +8.6212 to +19.2874 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 45.0644 to 61.6418 deg, Dec 8.6212 to 19.2874 deg
Loaded 4359 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): 3495 out of 3755 total matches.
Matched with Tycho-2 3755 out of 11518 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits:
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits (aperture=6.3)
Read 11553 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0659 to 61.6417 deg, Dec +8.6188 to +19.2794 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 45.0659 to 61.6417 deg, Dec 8.6188 to 19.2794 deg
Loaded 4354 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): 3503 out of 3754 total matches.
Matched with Tycho-2 3754 out of 11553 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits:
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
2.1 pix Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
3.0 pix fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
3.0 pix fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
2.1 pix wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
2.1 pix wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
Limiting magnitude estimates:
15.9 mag. Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
15.9 mag. Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
14.2 mag. fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
14.2 mag. fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.6HRczu1L8M (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits 860.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits'
This WCS solution (swarp) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=764, bad_region=0, passed=11518
Got 11518 stars (including 10741 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 11518 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 11412 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 11411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 11411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits (swarp) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits N_match=977 sigma_overall_arcsec=0.242 sigma_q1_arcsec=0.291 sigma_q2_arcsec=0.233 sigma_q3_arcsec=0.221 sigma_q4_arcsec=0.218 n_q1=265 n_q2=269 n_q3=245 n_q4=198 worst_quadrant_to_overall_ratio=1.204
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ZiGx6jp4vW (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits 860.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits'
This WCS solution (swarp) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=744, bad_region=0, passed=11553
Got 11553 stars (including 10798 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 11553 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 11432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 11434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 11434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits (swarp) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits N_match=976 sigma_overall_arcsec=0.268 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.259 sigma_q3_arcsec=0.229 sigma_q4_arcsec=0.239 n_q1=264 n_q2=270 n_q3=246 n_q4=196 worst_quadrant_to_overall_ratio=1.209
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PHfh5o1sAk (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_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.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_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=179, bad_region=0, passed=4057
Got 4057 stars (including 3873 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat
util/solve_plate_with_UCAC5 got 4057 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 491 to 549 (Dec 8.3 to 19.5)
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: 970 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 3997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 491 to 549 (Dec 8.3 to 19.5)
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: 970 matched stars entering correct_measured_positions(), 3997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 3997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=970 robust_rms=11.657 arcsec
SIP_REFIT: SIP order 3 trial: matched=970 robust_rms=0.324 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=970 robust_rms_before=0.891 arcsec robust_rms_before_corrected=0.270 arcsec robust_rms_after=0.324 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.270 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits N_match=970 sigma_overall_arcsec=0.280 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.363 sigma_q3_arcsec=0.257 sigma_q4_arcsec=0.247 n_q1=203 n_q2=220 n_q3=281 n_q4=266 worst_quadrant_to_overall_ratio=1.298
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits -region wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.mxInStmApi (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_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.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_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=179, bad_region=0, passed=4059
Got 4059 stars (including 3875 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat
util/solve_plate_with_UCAC5 got 4059 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 491 to 549 (Dec 8.3 to 19.5)
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: 969 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 3995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 3995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 3995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=969 robust_rms=11.371 arcsec
SIP_REFIT: SIP order 3 trial: matched=969 robust_rms=0.321 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=969 robust_rms_before=0.898 arcsec robust_rms_before_corrected=0.261 arcsec robust_rms_after=0.321 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.261 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits N_match=969 sigma_overall_arcsec=0.263 sigma_q1_arcsec=0.287 sigma_q2_arcsec=0.359 sigma_q3_arcsec=0.238 sigma_q4_arcsec=0.255 n_q1=205 n_q2=221 n_q3=281 n_q4=262 worst_quadrant_to_overall_ratio=1.363
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits -region wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat.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=Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits sigma_overall=0.242 worst_q_ratio=1.204
ref2=Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits sigma_overall=0.268 worst_q_ratio=1.209
new1=fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits sigma_overall=0.280 worst_q_ratio=1.298
new2=fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits sigma_overall=0.263 worst_q_ratio=1.363
reference average sigma_overall=0.255 worst_q_ratio=1.2065
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2_astrometric_residuals.png (977 matched stars from wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2_astrometric_residuals.png (976 matched stars from wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364_astrometric_residuals.png (970 matched stars from wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365_astrometric_residuals.png (969 matched stars from wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits'
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits'
Preparing the HTML report for the field Tau-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20595_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 20595_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
**** FOUND 03:54:23.55 +16:01:01.8 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 Tau-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.cat to cache
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
Creating symlink local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits exists and is non-empty
wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits exists and is non-empty
wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits exists and is non-empty
wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits (1st reference image)
verification OK: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:20.346 +13:59:54.22 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_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits (1st new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
Image size: 941.7'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:19.652 +13:57:39.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:33:20.346 +13:59:54.22
Second-epoch image center 03:33:19.652 +13:57:39.49
Angular distance between the image centers 0.0375 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits (2nd new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
Image size: 941.7'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:19.875 +13:57:41.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:33:20.346 +13:59:54.22
Second-epoch image center 03:33:19.875 +13:57:41.78
Angular distance between the image centers 0.0368 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 03:33:19.652 +13:57:39.49
Second-epoch second image center 03:33:19.875 +13:57:41.78
Angular distance between the image centers 0.00110 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00110 deg. (min. required shift: 0.00164 deg.)
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits &> /tmp/tmp.EzuPTga8rt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits &> /tmp/tmp.JWN0hlQLe2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits &> /tmp/tmp.SrKJyKDR2z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits &> /tmp/tmp.4mspenrbYn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat
The reference image (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits) and catalog (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat) found
'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat' -> 'wcsmag.cat'
Read 60881 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0645 to 61.6447 deg, Dec +8.6200 to +19.2873 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 45.0645 to 61.6447 deg, Dec 8.6200 to 19.2873 deg
Loaded 4360 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): 3155 out of 3759 total matches.
Matched with Tycho-2 3759 out of 60881 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.824000
a=0.000000 b=1.000000 c=22.824000
From vast_summary.log: estimated ref. image limiting mag.: -6.81
Updating vast_summary.log: Estimated ref. image limiting mag.: 16.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 16.01
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 60881 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0645 to 61.6447 deg, Dec +8.6200 to +19.2873 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 45.0645 to 61.6447 deg, Dec 8.6200 to 19.2873 deg
Loaded 4360 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): 3155 out of 3759 total matches.
Matched with Tycho-2 3759 out of 60881 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits:
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits (aperture=5.0)
Read 60861 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0659 to 61.6541 deg, Dec +8.6189 to +19.2796 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 45.0659 to 61.6541 deg, Dec 8.6189 to 19.2796 deg
Loaded 4359 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): 3151 out of 3757 total matches.
Matched with Tycho-2 3757 out of 60861 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits:
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 43 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
2.1 pix Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
2.8 pix fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
2.8 pix fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
2.1 pix wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
2.1 pix wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
Limiting magnitude estimates:
16.0 mag. Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
16.0 mag. Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
14.3 mag. fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
14.3 mag. fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.EzuPTga8rt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits 860.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits'
This WCS solution (swarp) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=3720, bad_region=3, passed=60861
Got 60861 stars (including 57045 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 60861 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 60410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 60408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 60408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits N_match=976 sigma_overall_arcsec=0.239 sigma_q1_arcsec=0.270 sigma_q2_arcsec=0.250 sigma_q3_arcsec=0.224 sigma_q4_arcsec=0.211 n_q1=270 n_q2=259 n_q3=245 n_q4=202 worst_quadrant_to_overall_ratio=1.132
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JWN0hlQLe2 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits 860.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits'
This WCS solution (swarp) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=3737, bad_region=5, passed=60834
Got 60834 stars (including 56991 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 60834 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 60381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 60382 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 60383 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits N_match=974 sigma_overall_arcsec=0.261 sigma_q1_arcsec=0.317 sigma_q2_arcsec=0.266 sigma_q3_arcsec=0.225 sigma_q4_arcsec=0.220 n_q1=266 n_q2=257 n_q3=248 n_q4=203 worst_quadrant_to_overall_ratio=1.214
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SrKJyKDR2z (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_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.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_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=560, bad_region=4, passed=21772
Got 21772 stars (including 21174 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat
util/solve_plate_with_UCAC5 got 21772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 491 to 549 (Dec 8.3 to 19.5)
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: 969 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 21417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 21418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 21418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits N_match=969 sigma_overall_arcsec=0.274 sigma_q1_arcsec=0.286 sigma_q2_arcsec=0.361 sigma_q3_arcsec=0.240 sigma_q4_arcsec=0.241 n_q1=206 n_q2=213 n_q3=284 n_q4=266 worst_quadrant_to_overall_ratio=1.320
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits -region wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4mspenrbYn (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_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.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_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=572, bad_region=4, passed=21986
Got 21986 stars (including 21372 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat
util/solve_plate_with_UCAC5 got 21986 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 491 to 549 (Dec 8.3 to 19.5)
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: 970 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 21653 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 491 to 549 (Dec 8.3 to 19.5)
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: 970 matched stars entering correct_measured_positions(), 21652 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 21652 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits N_match=970 sigma_overall_arcsec=0.272 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.380 sigma_q3_arcsec=0.243 sigma_q4_arcsec=0.247 n_q1=211 n_q2=213 n_q3=284 n_q4=262 worst_quadrant_to_overall_ratio=1.396
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits -region wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits.wcscat.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_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.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_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-47-48_20.00sec_-0.00C_LIGHTs_0364.fits
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.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_2026-07-26_CI_Tau-05-Q1b1x1_051307_TTUQ1b1x1_2872335_6Kvj7gKE/wcs_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365.fits
Preparing the HTML report for the field Tau-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:09:30.55 +13:36:17.3: 12.15 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:16:45.49 +15:39:49.2: 12.20 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:09:30.55 +13:36:17.3: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.00
Forced photometry filter REJECTED candidate at 03:09:30.55 +13:36:17.3: ref_mag=12.14 +/- 0.00 new_mean_mag=12.4295 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:16:45.49 +15:39:49.2: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter REJECTED candidate at 03:16:45.49 +15:39:49.2: ref_mag=12.20 +/- 0.01 new_mean_mag=12.3556 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:23:08.14 +16:35:51.3: 13.45 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:49:22.11 +17:49:47.7: 13.31 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:53:52.61 +15:11:43.1: 13.19 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:23:08.14 +16:35:51.3: 13.41 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:27:32.31 +16:40:07.9: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter REJECTED candidate at 03:23:08.14 +16:35:51.3: ref_mag=13.43 +/- 0.02 new_mean_mag=13.4061 delta=0.02 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:49:22.11 +17:49:47.7: 13.28 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:53:52.61 +15:11:43.1: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter REJECTED candidate at 03:49:22.11 +17:49:47.7: ref_mag=13.29 +/- 0.02 new_mean_mag=13.2499 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter REJECTED candidate at 03:53:52.61 +15:11:43.1: ref_mag=13.20 +/- 0.02 new_mean_mag=13.2016 delta=0.00 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:31:18.64 +17:58:04.3: 13.55 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:27:32.31 +16:40:07.9: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Forced photometry filter REJECTED candidate at 03:27:32.31 +16:40:07.9: ref_mag=13.62 +/- 0.02 new_mean_mag=13.4384 delta=0.18 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:08:03.60 +17:00:32.1: 13.51 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:40:57.51 +13:44:28.2: 13.55 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:31:18.64 +17:58:04.3: 13.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.02
Forced photometry filter REJECTED candidate at 03:31:18.64 +17:58:04.3: ref_mag=13.56 +/- 0.02 new_mean_mag=13.5621 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:12:13.95 +15:39:32.9: 16.58 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:08:03.60 +17:00:32.1: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Forced photometry filter REJECTED candidate at 03:08:03.60 +17:00:32.1: ref_mag=13.51 +/- 0.02 new_mean_mag=13.6577 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:40:57.51 +13:44:28.2: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Forced photometry filter REJECTED candidate at 03:40:57.51 +13:44:28.2: ref_mag=13.55 +/- 0.02 new_mean_mag=13.6115 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:06:26.67 +17:56:08.2: 16.47 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:54:50.77 +14:02:23.0: 16.62 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_stack2.fits at 03:59:34.20 +16:02:31.6: 16.51 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:12:13.95 +15:39:32.9: 16.53 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:54:50.77 +14:02:23.0: 16.59 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:06:26.67 +17:56:08.2: 16.44 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_stack2.fits at 03:59:34.20 +16:02:31.6: 16.42 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out75830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75880.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 23s
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 75322_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75322_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
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Considering the candidate 75401_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75401_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75410_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75410_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75411_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75411_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75420_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75420_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75456_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75456_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75473_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75473_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75493_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75493_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
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Considering the candidate 75517_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75517_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75581_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75581_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75590_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75590_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75612_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75612_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75636_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75636_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75647_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75647_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
**** FOUND 04:00:43.01 +18:12:31.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75661_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75661_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
**** FOUND 03:08:27.54 +10:46:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75670_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75670_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
**** FOUND 03:33:21.95 +13:45:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75671_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75671_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75676_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75676_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
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Considering the candidate 75680_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75680_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75681_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75681_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
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Considering the candidate 75683_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75683_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
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Considering the candidate 75693_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75693_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75719_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75719_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75725_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75725_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75729_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75729_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
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Considering the candidate 75730_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75730_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
**** FOUND 03:12:57.65 +17:08:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75731_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75731_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75742_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75742_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
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Considering the candidate 75752_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75752_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
**** FOUND 03:36:02.21 +16:29:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75756_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75756_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75757_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75757_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
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Considering the candidate 75803_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75803_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
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Considering the candidate 75813_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75813_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75830_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
Preparing report for the candidate 75830_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
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Considering the candidate 75845_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75845_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75859_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75859_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75866_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
Preparing report for the candidate 75866_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
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Considering the candidate 75870_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75870_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75871_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
Preparing report for the candidate 75871_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
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Considering the candidate 75878_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 75878_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 75880_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
Preparing report for the candidate 75880_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
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Considering the candidate 21229_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 21229_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks
**** FOUND 03:54:23.54 +16:01:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16012_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365
The candidate 16012_fd_Tau-05-Q1b1x1_2026-07-26_04-48-29_20.00sec_-0.00C_LIGHTs_0365 did not pass the final checks