This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 19.3566 2461271.8566 13.46 02:54:43.96 +18:36:53.1
159.47634 -35.36211 galactic Ari Second-epoch detections are separated by 1.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.419 Aurelia 0 -0 0 13.6 -0 0
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:54:43.96 +18:36:53.1: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:54:43.96 +18:36:53.1: 16.24 +/- 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 08 19.3566* 02 54 43.96 +18 36 53.1 13.5 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,2461271.8566,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260819.3566 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 19.3566 2461271.8566 14.02 02:56:22.17 +20:42:31.1
158.45380 -33.40739 galactic Ari Second-epoch detections are separated by 0.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.312 Pierretta -0 -0 0 14.4 -0 -0
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:22.17 +20:42:31.1: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:22.17 +20:42:31.1: 16.23 +/- 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 08 19.3566* 02 56 22.17 +20 42 31.1 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,2461271.8566,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260819.3566 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 19.3566 2461271.8566 14.11 02:57:26.56 +24:58:19.9
155.97545 -29.69498 galactic Ari Second-epoch detections are separated by 0.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.188 Menippe 0 -0 0 14.2 0 0
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:57:26.56 +24:58:19.9: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:57:26.56 +24:58:19.9: 16.24 +/- 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 08 19.3566* 02 57 26.56 +24 58 19.9 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
VARIABLE_NAME,2461271.8566,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260819.3566 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 19.3566 2461271.8566 14.69 03:02:22.11 +21:04:54.6
159.58514 -32.31225 galactic Ari Second-epoch detections are separated by 0.9" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.514 Armida 0 1 1 14.6 0 0
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:02:22.11 +21:04:54.6: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:02:22.11 +21:04:54.6: 16.16 +/- 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 08 19.3566* 03 02 22.11 +21 04 54.6 14.7 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,2461271.8566,14.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260819.3566 14.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 19.3566 2461271.8566 14.80 02:37:48.45 +19:06:52.6
154.93865 -37.05959 galactic Ari Second-epoch detections are separated by 1.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.248 Lameia 1 -0 1 15.0 -0 0
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:37:48.45 +19:06:52.6: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:37:48.45 +19:06:52.6: 16.20 +/- 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 08 19.3566* 02 37 48.45 +19 06 52.6 14.8 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,2461271.8566,14.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260819.3566 14.80CV 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: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
First image: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Last image: 2461271.85686890 19.08.2026 08:33:43.473 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
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: 25 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 8189
Objects passed selection criteria: 8162
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 2.0 2 4
Average stars detected per image: 6227.5
Average stars matched: 5734.25 (92.0795 %)
Memory usage VmPeak: 233640 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 19 03:52:10 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: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
First image: 2461049.66774773 09.01.2026 04:01:23.404 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Last image: 2461271.85686890 19.08.2026 08:33:43.473 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 93
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.22
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: 23 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 49687
Objects passed selection criteria: 49524
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 39128.8
Average stars matched: 35919 (91.797 %)
Memory usage VmPeak: 266556 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 19 03:53:39 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.cat to cache
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.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: 2461271.85642844
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits exists and is non-empty
wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits exists and is non-empty
wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits exists and is non-empty
wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (1st reference image)
verification OK: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Image size: 941.5'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: 02:46:09.152 +22:00:01.48 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_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits (1st new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:09.937 +22:00:13.75 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:46:09.152 +22:00:01.48
Second-epoch image center 02:46:09.937 +22:00:13.75
Angular distance between the image centers 0.0046 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits (2nd new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:10.999 +22:00:09.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:46:09.152 +22:00:01.48
Second-epoch image center 02:46:10.999 +22:00:09.91
Angular distance between the image centers 0.0075 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 02:46:09.937 +22:00:13.75
Second-epoch second image center 02:46:10.999 +22:00:09.91
Angular distance between the image centers 0.00424 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/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits &> /tmp/tmp.0CUSgo8Ntr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits &> /tmp/tmp.ycwhfViwgs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits &> /tmp/tmp.uw5VbumJn7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits &> /tmp/tmp.hYhBYjEjwk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
The reference image (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits) and catalog (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat) found
'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat' -> 'wcsmag.cat'
Read 9126 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8260 to 50.3988 deg, Dec +16.4916 to +27.2900 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 32.8260 to 50.3988 deg, Dec 16.4916 to 27.2900 deg
Loaded 5491 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): 4327 out of 4596 total matches.
Matched with Tycho-2 4596 out of 9126 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.948700
a=0.000000 b=1.000000 c=22.948700
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9126 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8260 to 50.3988 deg, Dec +16.4916 to +27.2900 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 32.8260 to 50.3988 deg, Dec 16.4916 to 27.2900 deg
Loaded 5491 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): 4327 out of 4596 total matches.
Matched with Tycho-2 4596 out of 9126 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (aperture=6.0)
Read 9076 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.7970 to 50.3462 deg, Dec +16.4915 to +27.2889 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 32.7970 to 50.3462 deg, Dec 16.4915 to 27.2889 deg
Loaded 5484 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): 4335 out of 4603 total matches.
Matched with Tycho-2 4603 out of 9076 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
2.0 pix Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
2.3 pix fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
2.4 pix fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Limiting magnitude estimates:
15.4 mag. Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
15.4 mag. Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
15.1 mag. fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
15.1 mag. fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.0CUSgo8Ntr (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=637, bad_region=2094, passed=9126
Got 9126 stars (including 6525 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 9126 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 7469 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4887 stars left (next iteration limit 5374)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits N_match=4887 sigma_overall_arcsec=0.306 sigma_q1_arcsec=0.373 sigma_q2_arcsec=0.300 sigma_q3_arcsec=0.273 sigma_q4_arcsec=0.257 n_q1=1673 n_q2=881 n_q3=1464 n_q4=869 worst_quadrant_to_overall_ratio=1.222
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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.ycwhfViwgs (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=628, bad_region=2087, passed=9076
Got 9076 stars (including 6485 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 9076 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 4888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 7417 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 7417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 7417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4889 stars left (next iteration limit 5376)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits N_match=4889 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.280 sigma_q4_arcsec=0.256 n_q1=1669 n_q2=883 n_q3=1466 n_q4=871 worst_quadrant_to_overall_ratio=1.216
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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.uw5VbumJn7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=422, bad_region=1887, passed=7365
Got 7365 stars (including 5152 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat
util/solve_plate_with_UCAC5 got 7365 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 4867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 5850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 5850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 5850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4869 stars left (next iteration limit 5353)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4869 robust_rms=6.949 arcsec worst_quadrant_rms=9.229 arcsec
SIP_REFIT: SIP order 3 trial: matched=4869 robust_rms=0.458 arcsec worst_quadrant_rms=0.572 arcsec
SIP_REFIT: SIP order 5 trial: matched=4869 robust_rms=0.364 arcsec worst_quadrant_rms=0.401 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4869 robust_rms_before=1.050 arcsec robust_rms_before_corrected=0.361 arcsec robust_rms_after=0.364 arcsec worst_quadrant_rms_before=0.381 worst_quadrant_rms_after=0.401
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.381 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits N_match=4869 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.413 sigma_q3_arcsec=0.410 sigma_q4_arcsec=0.358 n_q1=1485 n_q2=798 n_q3=1633 n_q4=953 worst_quadrant_to_overall_ratio=1.080
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits -region wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.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.hYhBYjEjwk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=402, bad_region=1862, passed=7417
Got 7417 stars (including 5240 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat
util/solve_plate_with_UCAC5 got 7417 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 5921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 5921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 5921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4866 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4866 robust_rms=6.908 arcsec worst_quadrant_rms=9.297 arcsec
SIP_REFIT: SIP order 3 trial: matched=4866 robust_rms=0.416 arcsec worst_quadrant_rms=0.521 arcsec
SIP_REFIT: SIP order 5 trial: matched=4866 robust_rms=0.333 arcsec worst_quadrant_rms=0.364 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4866 robust_rms_before=1.016 arcsec robust_rms_before_corrected=0.327 arcsec robust_rms_after=0.333 arcsec worst_quadrant_rms_before=0.344 worst_quadrant_rms_after=0.364
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.344 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits N_match=4866 sigma_overall_arcsec=0.336 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.361 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.318 n_q1=1470 n_q2=795 n_q3=1658 n_q4=943 worst_quadrant_to_overall_ratio=1.076
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits -region wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits to local_wcs_cache/
'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits' -> 'local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits'
Saving the final (post-refit) wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits to local_wcs_cache/
'wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits' -> 'local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits'
Saving the final (post-refit) wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits'
Saving the final (post-refit) wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits sigma_overall=0.306 worst_q_ratio=1.222
ref2=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits sigma_overall=0.300 worst_q_ratio=1.216
new1=fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits sigma_overall=0.382 worst_q_ratio=1.080
new2=fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits sigma_overall=0.336 worst_q_ratio=1.076
reference average sigma_overall=0.303 worst_q_ratio=1.219
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131_astrometric_residuals.png (4887 matched stars from wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132_astrometric_residuals.png (4889 matched stars from wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382_astrometric_residuals.png (4869 matched stars from wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383_astrometric_residuals.png (4866 matched stars from wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits'
Preparing the HTML report for the field Ari-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ari-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.cat to cache
SExtractor catalog cache: saved Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Creating symlink local_wcs_cache/wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits exists and is non-empty
wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits exists and is non-empty
wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits exists and is non-empty
wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (1st reference image)
verification OK: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Image size: 941.5'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: 02:46:09.152 +22:00:01.48 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_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits (1st new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:09.937 +22:00:13.75 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:46:09.152 +22:00:01.48
Second-epoch image center 02:46:09.937 +22:00:13.75
Angular distance between the image centers 0.0046 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
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# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits (2nd new image)
verification OK: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:46:10.999 +22:00:09.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:46:09.152 +22:00:01.48
Second-epoch image center 02:46:10.999 +22:00:09.91
Angular distance between the image centers 0.0075 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 02:46:09.937 +22:00:13.75
Second-epoch second image center 02:46:10.999 +22:00:09.91
Angular distance between the image centers 0.00424 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/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits &> /tmp/tmp.lEAPu37a8e
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits &> /tmp/tmp.oJiISHuQT1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits &> /tmp/tmp.Bg21KooJFp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits &> /tmp/tmp.dn1eeHzPCI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
Found non-empty wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
The reference image (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits) and catalog (wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat) found
'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat' -> 'wcsmag.cat'
Read 54392 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8053 to 50.3988 deg, Dec +16.4759 to +27.2958 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 32.8053 to 50.3988 deg, Dec 16.4759 to 27.2958 deg
Loaded 5502 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): 4040 out of 4639 total matches.
Matched with Tycho-2 4639 out of 54392 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.822300
a=0.000000 b=1.000000 c=22.822300
From vast_summary.log: estimated ref. image limiting mag.: -7.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.60
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 54392 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.8053 to 50.3988 deg, Dec +16.4759 to +27.2958 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 32.8053 to 50.3988 deg, Dec 16.4759 to 27.2958 deg
Loaded 5502 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): 4040 out of 4639 total matches.
Matched with Tycho-2 4639 out of 54392 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (aperture=4.6)
Read 54252 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 32.7970 to 50.3828 deg, Dec +16.4755 to +27.2950 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 32.7970 to 50.3828 deg, Dec 16.4755 to 27.2950 deg
Loaded 5501 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): 4037 out of 4639 total matches.
Matched with Tycho-2 4639 out of 54252 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Forced-photometry filter: calibrated wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -> calib.txt_param_ref_wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 59 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
1.9 pix Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
2.1 pix fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
2.2 pix fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Limiting magnitude estimates:
15.6 mag. Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
15.6 mag. Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
15.2 mag. fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
15.2 mag. fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.7 (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.lEAPu37a8e (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=2743, bad_region=10132, passed=54382
Got 54382 stars (including 41937 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 54382 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 46417 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 46417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 46417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4886 stars left (next iteration limit 5374)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits N_match=4886 sigma_overall_arcsec=0.293 sigma_q1_arcsec=0.353 sigma_q2_arcsec=0.280 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.251 n_q1=1667 n_q2=879 n_q3=1477 n_q4=863 worst_quadrant_to_overall_ratio=1.204
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.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.oJiISHuQT1 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits' -> 'wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS-calibrated image found: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
Checking if the catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits
WCS catalog name: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2775, bad_region=10166, passed=54247
Got 54247 stars (including 41735 good ones) from the SExtractor catalog wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 54247 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 4883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 46261 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 46261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 46261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4883 stars left (next iteration limit 5371)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits N_match=4883 sigma_overall_arcsec=0.290 sigma_q1_arcsec=0.351 sigma_q2_arcsec=0.274 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.240 n_q1=1655 n_q2=882 n_q3=1488 n_q4=858 worst_quadrant_to_overall_ratio=1.209
The image catalog is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits -region wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.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.Bg21KooJFp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1953, bad_region=7823, passed=42452
Got 42452 stars (including 33197 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat
util/solve_plate_with_UCAC5 got 42452 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 36556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 36556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 36556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4868 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4868 robust_rms=6.706 arcsec worst_quadrant_rms=8.458 arcsec
SIP_REFIT: SIP order 3 trial: matched=4868 robust_rms=0.446 arcsec worst_quadrant_rms=0.546 arcsec
SIP_REFIT: SIP order 5 trial: matched=4868 robust_rms=0.361 arcsec worst_quadrant_rms=0.395 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4868 robust_rms_before=1.028 arcsec robust_rms_before_corrected=0.356 arcsec robust_rms_after=0.361 arcsec worst_quadrant_rms_before=0.379 worst_quadrant_rms_after=0.395
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.379 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits N_match=4868 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.347 sigma_q2_arcsec=0.404 sigma_q3_arcsec=0.403 sigma_q4_arcsec=0.353 n_q1=1514 n_q2=796 n_q3=1601 n_q4=957 worst_quadrant_to_overall_ratio=1.071
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits -region wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.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.dn1eeHzPCI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Checking if the catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat corresponding to the image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
WCS catalog name: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1952, bad_region=7736, passed=42163
Got 42163 stars (including 32988 good ones) from the SExtractor catalog wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat
util/solve_plate_with_UCAC5 got 42163 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 36366 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 36366 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 36366 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4864 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4864 robust_rms=6.713 arcsec worst_quadrant_rms=8.568 arcsec
SIP_REFIT: SIP order 3 trial: matched=4864 robust_rms=0.408 arcsec worst_quadrant_rms=0.510 arcsec
SIP_REFIT: SIP order 5 trial: matched=4864 robust_rms=0.331 arcsec worst_quadrant_rms=0.355 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4864 robust_rms_before=1.004 arcsec robust_rms_before_corrected=0.324 arcsec robust_rms_after=0.331 arcsec worst_quadrant_rms_before=0.339 worst_quadrant_rms_after=0.355
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.339 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits N_match=4864 sigma_overall_arcsec=0.335 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.352 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.321 n_q1=1503 n_q2=797 n_q3=1605 n_q4=959 worst_quadrant_to_overall_ratio=1.051
The image catalog is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits -region wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.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_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-05_20.00sec_-0.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Ari-03-Q2b1x1_034919_TTUQ2b1x1_1915989_2dqqeykK/wcs_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383.fits
Preparing the HTML report for the field Ari-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:40:36.40 +23:51:21.1: 14.64 +/- 0.08 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:42:39.49 +20:05:52.3: 14.47 +/- 0.07 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:37:04.43 +21:04:42.3: 14.27 +/- 0.06 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:30:18.86 +25:21:10.1: 15.07 +/- 0.14 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:33:06.55 +25:59:24.3: 14.52 +/- 0.08 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:30:18.86 +25:21:10.1: 15.11 +/- 0.13 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:37:04.43 +21:04:42.3: 14.32 +/- 0.06 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:33:06.55 +25:59:24.3: 14.55 +/- 0.08 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.10
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:42:39.49 +20:05:52.3: 14.45 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.04
Forced photometry filter REJECTED candidate at 02:30:18.86 +25:21:10.1: ref_mag=15.09 +/- 0.10 new_mean_mag=14.9507 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:37:04.43 +21:04:42.3: ref_mag=14.29 +/- 0.04 new_mean_mag=14.5114 delta=-0.22 (need > 0.90)
Forced photometry reference-image weighted average: 14.53 +/- 0.06
Forced photometry reference-image weighted average: 14.46 +/- 0.05
Forced photometry filter REJECTED candidate at 02:33:06.55 +25:59:24.3: ref_mag=14.53 +/- 0.06 new_mean_mag=14.5850 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:42:39.49 +20:05:52.3: ref_mag=14.46 +/- 0.05 new_mean_mag=14.5646 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:40:36.40 +23:51:21.1: 14.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.05
Forced photometry filter REJECTED candidate at 02:40:36.40 +23:51:21.1: ref_mag=14.49 +/- 0.05 new_mean_mag=14.5900 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:54:43.96 +18:36:53.1: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:54:43.96 +18:36:53.1: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:56:22.17 +20:42:31.1: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:57:26.56 +24:58:19.9: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:56:22.17 +20:42:31.1: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:41:10.23 +23:37:01.0: 14.40 +/- 0.07 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:57:26.56 +24:58:19.9: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 03:02:22.11 +21:04:54.6: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:41:15.24 +18:11:13.7: 14.48 +/- 0.07 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:41:10.23 +23:37:01.0: 14.38 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.05
Forced photometry filter REJECTED candidate at 02:41:10.23 +23:37:01.0: ref_mag=14.39 +/- 0.05 new_mean_mag=14.3552 delta=0.04 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 03:02:22.11 +21:04:54.6: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:37:48.45 +19:06:52.6: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:41:15.24 +18:11:13.7: 14.60 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.06
Forced photometry filter REJECTED candidate at 02:41:15.24 +18:11:13.7: ref_mag=14.53 +/- 0.06 new_mean_mag=14.4823 delta=0.05 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:57:01.46 +20:56:16.9: 14.62 +/- 0.08 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:37:48.45 +19:06:52.6: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:31:26.78 +21:43:10.4: 15.10 +/- 0.13 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:57:01.46 +20:56:16.9: 14.77 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.06
Forced photometry filter REJECTED candidate at 02:57:01.46 +20:56:16.9: ref_mag=14.69 +/- 0.06 new_mean_mag=14.5753 delta=0.11 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:42:53.29 +25:13:37.8: 15.74 +/- 0.22 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-01-23_20.00sec_-15.00C_LIGHT_0131.fits at 02:33:57.04 +19:14:22.5: 15.69 +/- 0.21 detection
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:31:26.78 +21:43:10.4: 15.22 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.09
Forced photometry filter REJECTED candidate at 02:31:26.78 +21:43:10.4: ref_mag=15.15 +/- 0.09 new_mean_mag=14.9480 delta=0.21 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:42:53.29 +25:13:37.8: 15.62 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.67 +/- 0.15
Forced photometry filter REJECTED candidate at 02:42:53.29 +25:13:37.8: ref_mag=15.67 +/- 0.15 new_mean_mag=14.9946 delta=0.68 (need > 0.90)
Forced photometry on wcs_Ari-03-Q2b1x1_2026-01-08_22-02-16_20.00sec_-14.90C_LIGHT_0132.fits at 02:33:57.04 +19:14:22.5: 15.55 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.61 +/- 0.14
Forced photometry filter REJECTED candidate at 02:33:57.04 +19:14:22.5: ref_mag=15.61 +/- 0.14 new_mean_mag=15.1518 delta=0.46 (need > 0.90)
Adding exclusion_list_local.txt__out70820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74857.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 67538_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 67538_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
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Considering the candidate 67544_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 67544_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
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Considering the candidate 67546_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 67546_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
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Considering the candidate 67548_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 67548_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
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Considering the candidate 67549_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 67549_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
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Considering the candidate 67552_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 67552_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 68526_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 68526_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 70207_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 70207_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 70325_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 70325_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
**** FOUND 03:05:34.08 +25:15:31.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 70397_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 70397_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
**** FOUND 02:48:52.17 +25:12:16.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 70602_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 70602_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 70635_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 70635_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
**** FOUND 02:34:54.55 +22:25:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70693_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 70693_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 70775_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 70775_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 70820_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
Preparing report for the candidate 70820_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
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Considering the candidate 71253_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 71253_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
**** FOUND 02:47:30.26 +19:23:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71388_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 71388_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 71464_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 71464_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 71622_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 71622_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
**** FOUND 02:40:59.43 +19:58:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72182_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 72182_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 72364_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 72364_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 72511_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
Preparing report for the candidate 72511_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
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Considering the candidate 72598_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 72598_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 72621_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 72621_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 72724_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 72724_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 72863_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 72863_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 72897_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 72897_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 72982_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 72982_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 73009_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
Preparing report for the candidate 73009_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
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Considering the candidate 73075_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 73075_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 73247_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 73247_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 73250_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 73250_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 73306_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 73306_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 73359_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 73359_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
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Considering the candidate 73375_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 73375_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 73453_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 73453_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 73498_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 73498_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 73981_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 73981_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 74041_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
Preparing report for the candidate 74041_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
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Considering the candidate 74251_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 74251_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 74281_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 74281_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
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Considering the candidate 74506_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 74506_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 74528_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 74528_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 74586_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 74586_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 74694_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 74694_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 74824_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 74824_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 74857_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
Preparing report for the candidate 74857_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
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Considering the candidate 74975_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 74975_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 74985_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 74985_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 75038_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 75038_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 75252_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 75252_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
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Considering the candidate 75375_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 75375_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 75501_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 75501_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 75636_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 75636_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 75688_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 75688_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
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Considering the candidate 75692_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 75692_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 75746_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 75746_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 75853_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 75853_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks
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Considering the candidate 76030_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383
The candidate 76030_fd_Ari-03-Q2b1x1_2026-08-19_03-33-43_20.00sec_-0.00C_LIGHT_0383 did not pass the final checks