This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH
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 11 03.3062 2461347.8062 13.29 02:55:41.01 -00:50:57.7
176.74744 -50.26889 galactic Cet Second-epoch detections are separated by 3.0" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:55:41.01 -00:50:57.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 02:55:41.01 -00:50:57.7: 14.30 +/- 0.09 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 02:55:41.01 -00:50:57.7: 14.17 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.06
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 11 03.3062* 02 55 41.01 +00 50 57.7 13.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461347.8062,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261103.3062 13.29CV 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 11 03.3062 2461347.8062 12.83 02:59:19.30 +02:48:10.4
173.82623 -47.03675 galactic Cet Second-epoch detections are separated by 0.4" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.619 Triberga 0 -1 1 12.9 -0 0
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 02:59:19.30 +02:48:10.4: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 02:59:19.30 +02:48:10.4: 15.79 +/- 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 11 03.3062* 02 59 19.30 +02 48 10.4 12.8 U Cet 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,2461347.8062,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261103.3062 12.83CV 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 11 03.3062 2461347.8062 13.45 03:19:29.63 +03:01:11.1
178.60695 -43.28575 galactic Cet Second-epoch detections are separated by 0.8" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1104 Syringa 1 0 1 13.5 0 0
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:19:29.63 +03:01:11.1: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:19:29.63 +03:01:11.1: 16.03 +/- 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 11 03.3062* 03 19 29.63 +03 01 11.1 13.4 U Cet 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,2461347.8062,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261103.3062 13.45CV 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 11 03.3062 2461347.8062 13.39 03:51:04.54 -02:26:39.1
190.95205 -40.48004 galactic Eri Second-epoch detections are separated by 0.9" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.483 Seppina 0 1 1 13.5 0 -0
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:51:04.54 -02:26:39.1: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:51:04.54 -02:26:39.1: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 03.3062* 03 51 04.54 -02 26 39.1 13.4 U Eri 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,2461347.8062,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261103.3062 13.39CV 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 11 03.3062 2461347.8062 13.80 03:54:00.08 -07:00:15.7
196.60350 -42.31449 galactic Eri Second-epoch detections are separated by 7.6" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:54:00.08 -07:00:15.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:54:00.08 -07:00:15.7: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:54:00.08 -07:00:15.7: 15.56 +/- 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 11 03.3062* 03 54 00.08 -07 00 15.7 13.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461347.8062,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261103.3062 13.80CV 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
Mean magnitude and position on the discovery images:
2026 11 03.3062 2461347.8062 14.02 03:41:41.79 +01:44:03.4
184.72588 -39.89547 galactic Tau Second-epoch detections are separated by 0.5" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1403 Idelsonia -1 1 1 14.3 0 0
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:41:41.79 +01:44:03.4: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:41:41.79 +01:44:03.4: 15.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 11 03.3062* 03 41 41.79 +01 44 03.4 14.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461347.8062,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261103.3062 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.65583366 09.01.2026 03:44:14.028 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
First image: 2461049.65583366 09.01.2026 03:44:14.028 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Last image: 2461347.80651811 03.11.2026 07:21:13.165 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 3 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): 7246
Objects passed selection criteria: 7243
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 6691
Average stars matched: 6513.5 (97.3472 %)
Memory usage VmPeak: 233192 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 01:28:56 CST 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: 2461049.65583366 09.01.2026 03:44:14.028 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
First image: 2461049.65583366 09.01.2026 03:44:14.028 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Last image: 2461347.80651811 03.11.2026 07:21:13.165 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 38
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.16
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 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): 36527
Objects passed selection criteria: 36426
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 30781.2
Average stars matched: 29603.5 (96.1738 %)
Memory usage VmPeak: 259408 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 01:29:53 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
SExtractor catalog cache: saved Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.cat to cache
SExtractor catalog cache: saved Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461347.80579279
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits exists and is non-empty
wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits exists and is non-empty
wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits exists and is non-empty
wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (1st reference image)
verification OK: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:25:43.554 -02:00:23.97 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_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits (1st new image)
verification OK: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
Image size: 940.6'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 03:26:03.758 -01:59:40.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:25:43.554 -02:00:23.97
Second-epoch image center 03:26:03.758 -01:59:40.22
Angular distance between the image centers 0.0850 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits (2nd new image)
verification OK: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Image size: 940.6'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 03:26:00.996 -02:00:19.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:25:43.554 -02:00:23.97
Second-epoch image center 03:26:00.996 -02:00:19.77
Angular distance between the image centers 0.0726 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:26:03.758 -01:59:40.22
Second-epoch second image center 03:26:00.996 -02:00:19.77
Angular distance between the image centers 0.01590 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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits &> /tmp/tmp.cEPVaZgka6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits &> /tmp/tmp.urEEY9SMrn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits &> /tmp/tmp.hNK5XJHUHz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits &> /tmp/tmp.9sGfRycaly
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Calibrating the magnitude scale
Found non-empty wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
Found non-empty wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
The reference image (wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits) and catalog (wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat) found
'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat' -> 'wcsmag.cat'
Read 7165 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5324 to 59.3891 deg, Dec -7.3136 to +3.3057 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 43.5324 to 59.3891 deg, Dec -7.3136 to 3.3057 deg
Loaded 4649 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): 3753 out of 3933 total matches.
Matched with Tycho-2 3933 out of 7165 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.908300
a=0.000000 b=1.000000 c=22.908300
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7165 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5324 to 59.3891 deg, Dec -7.3136 to +3.3057 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 43.5324 to 59.3891 deg, Dec -7.3136 to 3.3057 deg
Loaded 4649 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): 3753 out of 3933 total matches.
Matched with Tycho-2 3933 out of 7165 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Forced-photometry filter: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits -> calib.txt_param_ref_wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (aperture=6.0)
Read 7098 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5101 to 59.3815 deg, Dec -7.3136 to +3.3024 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 43.5101 to 59.3815 deg, Dec -7.3136 to 3.3024 deg
Loaded 4649 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): 3745 out of 3917 total matches.
Matched with Tycho-2 3917 out of 7098 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Forced-photometry filter: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits -> calib.txt_param_ref_wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 20 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
2.0 pix Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
5.4 pix fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
5.4 pix fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Limiting magnitude estimates:
15.5 mag. Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
15.5 mag. Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
14.6 mag. fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
14.6 mag. fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 12.0 (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.cEPVaZgka6 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits' -> 'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS-calibrated image found: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Checking if the catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS catalog name: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=532, bad_region=0, passed=7165
Got 7165 stars (including 6616 good ones) from the SExtractor catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
util/solve_plate_with_UCAC5 got 7165 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 4894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 7165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 7165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 7165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4894 stars left (next iteration limit 5383)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits N_match=4894 sigma_overall_arcsec=0.259 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.250 sigma_q3_arcsec=0.231 sigma_q4_arcsec=0.224 n_q1=1232 n_q2=1175 n_q3=1357 n_q4=1130 worst_quadrant_to_overall_ratio=1.300
WCS_HEADER_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits selection=current_pairs N_selected=4894 N_valid=4894 bias_ra_arcsec=-0.008 bias_dec_arcsec=-0.000 median_sep_arcsec=0.222 p95_sep_arcsec=0.733 n_q1=1232 n_q2=1175 n_q3=1357 n_q4=1130 occupied_cells_4x4=16/16
The image catalog is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits -region wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.urEEY9SMrn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits' -> 'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS_IMAGE_NAME=wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS-calibrated image found: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Checking if the catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits alredy exist and is non-empty...
Catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS catalog name: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=523, bad_region=0, passed=7098
Got 7098 stars (including 6565 good ones) from the SExtractor catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat
util/solve_plate_with_UCAC5 got 7098 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 4896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 7098 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7098 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7098 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4895 stars left (next iteration limit 5385)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits N_match=4895 sigma_overall_arcsec=0.263 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.255 sigma_q3_arcsec=0.237 sigma_q4_arcsec=0.230 n_q1=1233 n_q2=1170 n_q3=1359 n_q4=1133 worst_quadrant_to_overall_ratio=1.303
WCS_HEADER_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits selection=current_pairs N_selected=4895 N_valid=4895 bias_ra_arcsec=-0.002 bias_dec_arcsec=-0.001 median_sep_arcsec=0.222 p95_sep_arcsec=0.749 n_q1=1233 n_q2=1170 n_q3=1359 n_q4=1133 occupied_cells_4x4=16/16
The image catalog is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits -region wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.hNK5XJHUHz (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_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.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_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
WCS_IMAGE_NAME=wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
WCS-calibrated image found: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
Checking if the catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
WCS catalog name: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=264, bad_region=0, passed=6315
Got 6315 stars (including 6051 good ones) from the SExtractor catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat
util/solve_plate_with_UCAC5 got 6315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.6'
Seting catalog search parameters based on the expected field of view 940.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013064 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010451 (37.6 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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 6315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 6315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 6315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4908 stars left (next iteration limit 5397)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4908 robust_rms=13.079 arcsec worst_region_rms=27.662 arcsec outer_annulus_rms=27.662 arcsec
SIP_REFIT: SIP order 3 trial: matched=4908 robust_rms=0.542 arcsec worst_region_rms=0.899 arcsec outer_annulus_rms=0.899 arcsec
SIP_REFIT: SIP order 5 trial: matched=4908 robust_rms=0.460 arcsec worst_region_rms=0.808 arcsec outer_annulus_rms=0.808 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4908 robust_rms_before=0.881 arcsec robust_rms_before_corrected=0.460 arcsec robust_rms_after=0.460 arcsec worst_region_rms_before=0.833 worst_region_rms_after=0.808 outer_annulus_rms_before=1.477 outer_annulus_rms_after=0.808
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.833 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits worst_region_rms_kept=0.833 arcsec robust_rms_kept=0.460 arcsec matched=4908
WCS_QUALITY_DIAG: file=fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits N_match=4908 sigma_overall_arcsec=0.448 sigma_q1_arcsec=0.569 sigma_q2_arcsec=0.529 sigma_q3_arcsec=0.370 sigma_q4_arcsec=0.388 n_q1=1067 n_q2=1275 n_q3=1293 n_q4=1273 worst_quadrant_to_overall_ratio=1.269
WCS_HEADER_DIAG: file=fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits selection=current_pairs N_selected=4908 N_valid=4908 bias_ra_arcsec=-0.037 bias_dec_arcsec=0.101 median_sep_arcsec=0.759 p95_sep_arcsec=2.105 n_q1=1067 n_q2=1275 n_q3=1293 n_q4=1273 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits -region wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.9sGfRycaly (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_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.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_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
WCS_IMAGE_NAME=wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
WCS-calibrated image found: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Checking if the catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
WCS catalog name: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=264, bad_region=0, passed=6392
Got 6392 stars (including 6127 good ones) from the SExtractor catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat
util/solve_plate_with_UCAC5 got 6392 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.6'
Seting catalog search parameters based on the expected field of view 940.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013064 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010451 (37.6 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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4907 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 6392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 6392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 6392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4902 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4902 robust_rms=12.947 arcsec worst_region_rms=27.853 arcsec outer_annulus_rms=27.853 arcsec
SIP_REFIT: SIP order 3 trial: matched=4902 robust_rms=0.536 arcsec worst_region_rms=0.892 arcsec outer_annulus_rms=0.892 arcsec
SIP_REFIT: SIP order 5 trial: matched=4902 robust_rms=0.453 arcsec worst_region_rms=0.768 arcsec outer_annulus_rms=0.768 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4902 robust_rms_before=0.837 arcsec robust_rms_before_corrected=0.471 arcsec robust_rms_after=0.453 arcsec worst_region_rms_before=0.835 worst_region_rms_after=0.768 outer_annulus_rms_before=1.477 outer_annulus_rms_after=0.768
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.835 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits worst_region_rms_kept=0.835 arcsec robust_rms_kept=0.471 arcsec matched=4902
WCS_QUALITY_DIAG: file=fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits N_match=4902 sigma_overall_arcsec=0.441 sigma_q1_arcsec=0.568 sigma_q2_arcsec=0.549 sigma_q3_arcsec=0.358 sigma_q4_arcsec=0.357 n_q1=1066 n_q2=1283 n_q3=1285 n_q4=1268 worst_quadrant_to_overall_ratio=1.287
WCS_HEADER_DIAG: file=fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits selection=current_pairs N_selected=4902 N_valid=4902 bias_ra_arcsec=-0.040 bias_dec_arcsec=0.101 median_sep_arcsec=0.720 p95_sep_arcsec=2.157 n_q1=1066 n_q2=1283 n_q3=1285 n_q4=1268 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits -region wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits to local_wcs_cache/
'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits' -> 'local_wcs_cache/wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits'
Saving the final (post-refit) wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits to local_wcs_cache/
'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits' -> 'local_wcs_cache/wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits'
Saving the final (post-refit) wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits to local_wcs_cache/
'wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits' -> 'local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits'
Saving the final (post-refit) wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits to local_wcs_cache/
'wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits' -> 'local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits sigma_overall=0.259 worst_q_ratio=1.300
ref2=Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits sigma_overall=0.263 worst_q_ratio=1.303
new1=fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits sigma_overall=0.448 worst_q_ratio=1.269
new2=fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits sigma_overall=0.441 worst_q_ratio=1.287
reference average sigma_overall=0.261 worst_q_ratio=1.3015
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115_astrometric_residuals.png (4894 matched stars from wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116_astrometric_residuals.png (4895 matched stars from wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333_astrometric_residuals.png (4908 matched stars from wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334_astrometric_residuals.png (4902 matched stars from wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits'
Saving fully-calibrated image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits'
Preparing the HTML report for the field Eri-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:45:21.13 -00:56:48.7: 12.59 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:42:19.23 +00:34:10.3: 12.52 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:38:37.54 +02:55:37.3: 12.48 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:32:38.21 +03:01:32.3: 12.58 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:27:35.54 -00:15:45.2: 12.37 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:28:09.66 -01:18:05.6: 12.52 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:09:50.74 +01:40:18.3: 12.47 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:45:16.88 -01:47:43.9: 12.14 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:24:03.60 -00:25:28.5: 12.37 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:26:09.31 +00:54:57.0: 12.44 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:38:37.54 +02:55:37.3: 12.47 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:28:09.66 -01:18:05.6: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter REJECTED candidate at 03:38:37.54 +02:55:37.3: ref_mag=12.48 +/- 0.01 new_mean_mag=12.2039 delta=0.27 (need > 0.90)
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter REJECTED candidate at 03:28:09.66 -01:18:05.6: ref_mag=12.53 +/- 0.01 new_mean_mag=12.0288 delta=0.50 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:09:50.74 +01:40:18.3: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 03:09:50.74 +01:40:18.3: ref_mag=12.49 +/- 0.01 new_mean_mag=12.1775 delta=0.31 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:27:35.54 -00:15:45.2: 12.38 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:45:16.88 -01:47:43.9: 12.10 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:45:21.13 -00:56:48.7: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:24:03.60 -00:25:28.5: 12.42 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 03:45:16.88 -01:47:43.9: ref_mag=12.12 +/- 0.01 new_mean_mag=11.9717 delta=0.14 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:26:09.31 +00:54:57.0: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:32:38.21 +03:01:32.3: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter REJECTED candidate at 03:24:03.60 -00:25:28.5: ref_mag=12.39 +/- 0.01 new_mean_mag=12.0778 delta=0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:27:35.54 -00:15:45.2: ref_mag=12.38 +/- 0.01 new_mean_mag=12.1374 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 03:45:21.13 -00:56:48.7: ref_mag=12.62 +/- 0.01 new_mean_mag=12.1362 delta=0.48 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:42:19.23 +00:34:10.3: 12.49 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 03:26:09.31 +00:54:57.0: ref_mag=12.44 +/- 0.01 new_mean_mag=12.2172 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter REJECTED candidate at 03:32:38.21 +03:01:32.3: ref_mag=12.61 +/- 0.01 new_mean_mag=12.2506 delta=0.36 (need > 0.90)
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter REJECTED candidate at 03:42:19.23 +00:34:10.3: ref_mag=12.50 +/- 0.01 new_mean_mag=12.1161 delta=0.39 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:49:23.73 +02:32:28.5: 12.42 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:01:30.85 +01:42:28.0: 12.63 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:35:43.95 +01:01:36.5: 12.45 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:34:35.33 -01:15:13.8: 12.42 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:41:20.74 +01:08:07.0: 12.49 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:26:21.58 +01:09:26.1: 12.53 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:46:40.12 +02:35:26.2: 12.55 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:39:38.84 +00:42:47.1: 12.50 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:26:34.31 +02:21:15.5: 12.45 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:10:09.38 +02:55:30.1: 12.59 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:34:35.33 -01:15:13.8: 12.37 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:26:21.58 +01:09:26.1: 12.48 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:46:40.12 +02:35:26.2: 12.54 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:01:30.85 +01:42:28.0: 12.65 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:35:43.95 +01:01:36.5: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:10:09.38 +02:55:30.1: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:26:34.31 +02:21:15.5: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:39:38.84 +00:42:47.1: 12.41 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 03:46:40.12 +02:35:26.2: ref_mag=12.55 +/- 0.01 new_mean_mag=12.3355 delta=0.21 (need > 0.90)
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter REJECTED candidate at 03:34:35.33 -01:15:13.8: ref_mag=12.39 +/- 0.01 new_mean_mag=12.2481 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:26:21.58 +01:09:26.1: ref_mag=12.50 +/- 0.01 new_mean_mag=12.2824 delta=0.22 (need > 0.90)
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:49:23.73 +02:32:28.5: 12.47 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 03:35:43.95 +01:01:36.5: ref_mag=12.46 +/- 0.01 new_mean_mag=12.3055 delta=0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:01:30.85 +01:42:28.0: ref_mag=12.64 +/- 0.01 new_mean_mag=12.2942 delta=0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:10:09.38 +02:55:30.1: ref_mag=12.59 +/- 0.01 new_mean_mag=12.3092 delta=0.28 (need > 0.90)
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 03:26:34.31 +02:21:15.5: ref_mag=12.47 +/- 0.01 new_mean_mag=12.2395 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:39:38.84 +00:42:47.1: ref_mag=12.45 +/- 0.01 new_mean_mag=12.2825 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 03:49:23.73 +02:32:28.5: ref_mag=12.44 +/- 0.01 new_mean_mag=12.2243 delta=0.22 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:41:20.74 +01:08:07.0: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter REJECTED candidate at 03:41:20.74 +01:08:07.0: ref_mag=12.51 +/- 0.01 new_mean_mag=12.2596 delta=0.25 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20408_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20408_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
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Considering the candidate 20413_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20413_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
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Considering the candidate 20418_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20418_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
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Considering the candidate 20428_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20428_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20432_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20432_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
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Considering the candidate 20435_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20435_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
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Considering the candidate 20436_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20436_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
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Considering the candidate 20442_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20442_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20446_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20446_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
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Considering the candidate 20448_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20448_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20451_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20451_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20453_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20453_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20455_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20455_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20456_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20456_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20457_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20457_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20459_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20459_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20460_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20460_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20461_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20461_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20462_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20462_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20464_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 20464_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Eri-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
SExtractor catalog cache: saved Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.cat to cache
SExtractor catalog cache: saved Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Creating symlink local_wcs_cache/wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Creating symlink local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
Creating symlink local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Checking 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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits exists and is non-empty
wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits exists and is non-empty
wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits exists and is non-empty
wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (1st reference image)
verification OK: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:25:43.554 -02:00:23.97 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_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits (1st new image)
verification OK: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
Image size: 940.6'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 03:26:03.758 -01:59:40.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:25:43.554 -02:00:23.97
Second-epoch image center 03:26:03.758 -01:59:40.22
Angular distance between the image centers 0.0850 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits (2nd new image)
verification OK: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Image size: 940.6'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 03:26:00.996 -02:00:19.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:25:43.554 -02:00:23.97
Second-epoch image center 03:26:00.996 -02:00:19.77
Angular distance between the image centers 0.0726 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:26:03.758 -01:59:40.22
Second-epoch second image center 03:26:00.996 -02:00:19.77
Angular distance between the image centers 0.01590 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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits &> /tmp/tmp.vtcH4IJ4v9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits &> /tmp/tmp.8jhrTu035L
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits &> /tmp/tmp.BLK6rQrbb8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits &> /tmp/tmp.SXYtd77I2n
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Calibrating the magnitude scale
Found non-empty wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
Found non-empty wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
The reference image (wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits) and catalog (wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat) found
'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat' -> 'wcsmag.cat'
Read 38842 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5260 to 59.3942 deg, Dec -7.3141 to +3.3249 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 43.5260 to 59.3942 deg, Dec -7.3141 to 3.3249 deg
Loaded 4661 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): 3618 out of 4007 total matches.
Matched with Tycho-2 4007 out of 38842 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.808100
a=0.000000 b=1.000000 c=22.808100
From vast_summary.log: estimated ref. image limiting mag.: -7.16
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.65
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.65
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 38842 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5260 to 59.3942 deg, Dec -7.3141 to +3.3249 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 43.5260 to 59.3942 deg, Dec -7.3141 to 3.3249 deg
Loaded 4661 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): 3618 out of 4007 total matches.
Matched with Tycho-2 4007 out of 38842 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Forced-photometry filter: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits -> calib.txt_param_ref_wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (aperture=4.8)
Read 38876 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5102 to 59.3884 deg, Dec -7.3192 to +3.3177 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 43.5102 to 59.3884 deg, Dec -7.3192 to 3.3177 deg
Loaded 4658 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): 3627 out of 4001 total matches.
Matched with Tycho-2 4001 out of 38876 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Forced-photometry filter: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits -> calib.txt_param_ref_wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 32 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
1.9 pix Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
4.9 pix fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
4.8 pix fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Limiting magnitude estimates:
15.6 mag. Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
15.6 mag. Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
15.0 mag. fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
15.0 mag. fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 13.9 (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.vtcH4IJ4v9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits' -> 'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS-calibrated image found: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Checking if the catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS catalog name: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1673, bad_region=4, passed=38833
Got 38833 stars (including 37092 good ones) from the SExtractor catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
util/solve_plate_with_UCAC5 got 38833 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4901 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits N_match=4901 sigma_overall_arcsec=0.252 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.251 sigma_q3_arcsec=0.224 sigma_q4_arcsec=0.222 n_q1=1231 n_q2=1165 n_q3=1361 n_q4=1144 worst_quadrant_to_overall_ratio=1.275
WCS_HEADER_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits selection=current_pairs N_selected=4901 N_valid=4901 bias_ra_arcsec=-0.002 bias_dec_arcsec=0.002 median_sep_arcsec=0.216 p95_sep_arcsec=0.732 n_q1=1231 n_q2=1165 n_q3=1361 n_q4=1144 occupied_cells_4x4=16/16
The image catalog is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits -region wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.8jhrTu035L (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits' -> 'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS_IMAGE_NAME=wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS-calibrated image found: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Checking if the catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits alredy exist and is non-empty...
Catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS catalog name: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1668, bad_region=4, passed=38854
Got 38854 stars (including 37119 good ones) from the SExtractor catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat
util/solve_plate_with_UCAC5 got 38854 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4901 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits N_match=4901 sigma_overall_arcsec=0.256 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.258 sigma_q3_arcsec=0.229 sigma_q4_arcsec=0.224 n_q1=1233 n_q2=1169 n_q3=1356 n_q4=1143 worst_quadrant_to_overall_ratio=1.280
WCS_HEADER_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits selection=current_pairs N_selected=4901 N_valid=4901 bias_ra_arcsec=0.000 bias_dec_arcsec=0.000 median_sep_arcsec=0.215 p95_sep_arcsec=0.730 n_q1=1233 n_q2=1169 n_q3=1356 n_q4=1143 occupied_cells_4x4=16/16
The image catalog is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits -region wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.BLK6rQrbb8 (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_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.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_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
WCS_IMAGE_NAME=wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
WCS-calibrated image found: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
Checking if the catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
WCS catalog name: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=1628, bad_region=48, passed=23197
Got 23197 stars (including 21510 good ones) from the SExtractor catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat
util/solve_plate_with_UCAC5 got 23197 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.6'
Seting catalog search parameters based on the expected field of view 940.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013064 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010451 (37.6 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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 4885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 23197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 412 to 469 (Dec -7.5 to 3.5)
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(), 23197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 23197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4886 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.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=4886 robust_rms=13.121 arcsec worst_region_rms=27.630 arcsec outer_annulus_rms=27.630 arcsec
SIP_REFIT: SIP order 3 trial: matched=4886 robust_rms=0.543 arcsec worst_region_rms=0.893 arcsec outer_annulus_rms=0.893 arcsec
SIP_REFIT: SIP order 5 trial: matched=4886 robust_rms=0.459 arcsec worst_region_rms=0.769 arcsec outer_annulus_rms=0.769 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4886 robust_rms_before=0.891 arcsec robust_rms_before_corrected=0.458 arcsec robust_rms_after=0.459 arcsec worst_region_rms_before=0.788 worst_region_rms_after=0.769 outer_annulus_rms_before=1.492 outer_annulus_rms_after=0.769
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.788 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits worst_region_rms_kept=0.788 arcsec robust_rms_kept=0.458 arcsec matched=4886
WCS_QUALITY_DIAG: file=fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits N_match=4886 sigma_overall_arcsec=0.448 sigma_q1_arcsec=0.560 sigma_q2_arcsec=0.533 sigma_q3_arcsec=0.368 sigma_q4_arcsec=0.394 n_q1=1048 n_q2=1251 n_q3=1291 n_q4=1296 worst_quadrant_to_overall_ratio=1.251
WCS_HEADER_DIAG: file=fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits selection=current_pairs N_selected=4886 N_valid=4886 bias_ra_arcsec=-0.023 bias_dec_arcsec=0.071 median_sep_arcsec=0.767 p95_sep_arcsec=2.162 n_q1=1048 n_q2=1251 n_q3=1291 n_q4=1296 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits -region wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.SXYtd77I2n (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_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.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_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
WCS_IMAGE_NAME=wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
WCS-calibrated image found: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Checking if the catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
WCS catalog name: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=64, blended=1644, bad_region=48, passed=23474
Got 23474 stars (including 21770 good ones) from the SExtractor catalog wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat
util/solve_plate_with_UCAC5 got 23474 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.6'
Seting catalog search parameters based on the expected field of view 940.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013064 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010451 (37.6 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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 4885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 23474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4890 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(), 23474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 23474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4886 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.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=4886 robust_rms=12.998 arcsec worst_region_rms=27.779 arcsec outer_annulus_rms=27.779 arcsec
SIP_REFIT: SIP order 3 trial: matched=4886 robust_rms=0.533 arcsec worst_region_rms=0.878 arcsec outer_annulus_rms=0.878 arcsec
SIP_REFIT: SIP order 5 trial: matched=4886 robust_rms=0.449 arcsec worst_region_rms=0.745 arcsec outer_annulus_rms=0.745 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4886 robust_rms_before=0.843 arcsec robust_rms_before_corrected=0.474 arcsec robust_rms_after=0.449 arcsec worst_region_rms_before=0.819 worst_region_rms_after=0.745 outer_annulus_rms_before=1.475 outer_annulus_rms_after=0.745
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.819 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits worst_region_rms_kept=0.819 arcsec robust_rms_kept=0.474 arcsec matched=4886
WCS_QUALITY_DIAG: file=fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits N_match=4886 sigma_overall_arcsec=0.448 sigma_q1_arcsec=0.572 sigma_q2_arcsec=0.544 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.370 n_q1=1049 n_q2=1247 n_q3=1290 n_q4=1300 worst_quadrant_to_overall_ratio=1.277
WCS_HEADER_DIAG: file=fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits selection=current_pairs N_selected=4886 N_valid=4886 bias_ra_arcsec=-0.017 bias_dec_arcsec=0.074 median_sep_arcsec=0.729 p95_sep_arcsec=2.160 n_q1=1049 n_q2=1247 n_q3=1290 n_q4=1300 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits -region wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.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_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-20-10_20.00sec_-0.00C_LIGHTs_0333.fits
Saving fully-calibrated image wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.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_2026-11-03_CI_Eri-01-Q1b1x1_012201_TTUQ1b1x1_416015_LpywEGUH/wcs_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334.fits
Preparing the HTML report for the field Eri-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:51:04.54 -02:26:39.1: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 02:54:33.41 -06:05:26.9: 13.17 +/- 0.03 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:54:00.08 -07:00:15.7: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 02:59:19.30 +02:48:10.4: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:12:35.64 -06:45:28.7: 12.76 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:19:29.63 +03:01:11.1: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:19:27.30 -02:30:36.8: 14.07 +/- 0.05 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:41:41.79 +01:44:03.4: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 02:55:41.01 -00:50:57.7: 14.30 +/- 0.09 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:54:00.08 -07:00:15.7: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 02:59:19.30 +02:48:10.4: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 02:54:33.41 -06:05:26.9: 12.93 +/- 0.03 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:41:41.79 +01:44:03.4: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:19:29.63 +03:01:11.1: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:12:35.64 -06:45:28.7: 12.81 +/- 0.02 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:51:04.54 -02:26:39.1: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:19:27.30 -02:30:36.8: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter REJECTED candidate at 02:54:33.41 -06:05:26.9: ref_mag=13.03 +/- 0.02 new_mean_mag=13.2338 delta=-0.20 (need > 0.90)
Forced photometry reference-image weighted average: 14.14 +/- 0.04
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter REJECTED candidate at 03:12:35.64 -06:45:28.7: ref_mag=12.79 +/- 0.01 new_mean_mag=12.7095 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:19:27.30 -02:30:36.8: ref_mag=14.14 +/- 0.04 new_mean_mag=13.7867 delta=0.35 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 02:55:41.01 -00:50:57.7: 14.17 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.06
Forced photometry filter KEPT candidate at 02:55:41.01 -00:50:57.7: ref_mag=14.23 +/- 0.06 new_mean_mag=13.2900 delta=0.94 (need > 0.90)
Adding exclusion_list_local.txt__out52737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53406.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 426s
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: 4s
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Considering the candidate 52690_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 52690_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
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Considering the candidate 52731_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 52731_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
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Considering the candidate 52737_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
Preparing report for the candidate 52737_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
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Considering the candidate 52743_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 52743_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
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Considering the candidate 52970_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
Preparing report for the candidate 52970_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
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Considering the candidate 53184_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
Preparing report for the candidate 53184_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
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Considering the candidate 53224_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
Preparing report for the candidate 53224_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
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Considering the candidate 53393_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
Preparing report for the candidate 53393_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
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Considering the candidate 53406_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
Preparing report for the candidate 53406_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
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Considering the candidate 28839_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 28839_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 15103_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 15103_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:18:23.08 -00:55:56.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32562_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 32562_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:35:57.18 -05:07:30.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 16072_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 16072_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:12:47.12 -01:11:53.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32840_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 32840_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:30:36.92 -05:04:27.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 38796_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 38796_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:39:38.15 -03:23:37.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 09690_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 09690_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:36:51.76 +00:23:46.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 37595_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 37595_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:11:18.96 -03:48:42.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 30444_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 30444_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:16:21.84 -05:43:49.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 24298_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 24298_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:48:47.19 -07:00:51.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 25505_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 25505_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:53:08.42 -06:38:03.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 29790_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 29790_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:16:00.96 -05:55:07.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 25314_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 25314_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:29:38.96 -06:48:18.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 30651_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 30651_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:39:00.95 -05:37:40.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 26453_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 26453_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:02:09.45 -06:29:45.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32119_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 32119_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:40:38.09 -05:12:38.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 22428_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 22428_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:00:51.06 -02:52:45.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31401_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 31401_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:52:41.67 -05:21:43.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 23113_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 23113_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:54:17.41 -02:57:18.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21050_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 21050_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 02:59:41.26 -02:27:57.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 29062_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 29062_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 03:06:33.76 -06:05:19.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31039_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 31039_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
**** FOUND 02:56:37.44 -03:42:48.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 22212_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334
The candidate 22212_fd_Eri-01-Q1b1x1_2026-11-03_01-21-13_20.00sec_-0.00C_LIGHTs_0334 did not pass the final checks
