This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp
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 06 02.1473 2461193.6473 13.26 10:47:29.22 +34:10:23.2
190.42617 62.54337 galactic LMi Second-epoch detections are separated by 2.3" and 0.8 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 | 10:47:29.22 +34:10:23.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 10:47:29.22 +34:10:23.2: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 10:47:29.22 +34:10:23.2: 16.17 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461193.6473,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260602.1473 13.26CV 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 06 02.1473 2461193.6473 13.51 10:49:09.19 +30:15:19.8
198.96069 63.08152 galactic LMi Second-epoch detections are separated by 7.9" and 0.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:49:09.19 +30:15:19.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 10:49:09.19 +30:15:19.8: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 10:49:09.19 +30:15:19.8: 16.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461193.6473,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260602.1473 13.51CV 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 06 02.1473 2461193.6473 13.60 11:08:23.37 +25:51:26.9
210.20823 66.94821 galactic Leo Second-epoch detections are separated by 7.5" and 0.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:08:23.37 +25:51:26.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 11:08:23.37 +25:51:26.9: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 11:08:23.37 +25:51:26.9: 16.21 +/- 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 06 02.1473* 11 08 23.37 +25 51 26.9 13.6 U Leo 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,2461193.6473,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260602.1473 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 02.1473 2461193.6473 13.78 11:10:38.17 +30:54:30.4
197.16248 67.69064 galactic UMa Second-epoch detections are separated by 7.5" and 0.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:10:38.17 +30:54:30.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 11:10:38.17 +30:54:30.4: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 11:10:38.17 +30:54:30.4: 16.27 +/- 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 06 02.1473* 11 10 38.17 +30 54 30.4 13.8 U UMa 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,2461193.6473,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260602.1473 13.78CV 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 06 02.1473 2461193.6473 13.76 11:08:02.11 +29:28:39.5
200.92726 67.16557 galactic UMa Second-epoch detections are separated by 2.0" and 0.7 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 | 11:08:02.11 +29:28:39.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 11:08:02.11 +29:28:39.5: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 11:08:02.11 +29:28:39.5: 16.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 02.1473* 11 08 02.11 +29 28 39.5 13.8 U UMa 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,2461193.6473,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260602.1473 13.76CV 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: 2461093.81001216 22.02.2026 07:26:15.051 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
First image: 2461093.81001216 22.02.2026 07:26:15.051 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
Last image: 2461193.64750139 02.06.2026 03:32:14.120 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
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: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4985
Objects passed selection criteria: 4953
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 3095.75
Average stars matched: 2920.75 (94.3471 %)
Memory usage VmPeak: 111204 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 1 15:05:05 CDT 2026
VaST build number 1.0rc89-85-g6dfb2809
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 1 22:44:07 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.81001216 22.02.2026 07:26:15.051 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
First image: 2461093.81001216 22.02.2026 07:26:15.051 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
Last image: 2461193.64750139 02.06.2026 03:32:14.120 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 70
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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: 11 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 26241
Objects passed selection criteria: 26169
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 17725.5
Average stars matched: 16550.2 (93.3697 %)
Memory usage VmPeak: 129656 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 1 15:05:05 CDT 2026
VaST build number 1.0rc89-85-g6dfb2809
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 1 22:45:42 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
SExtractor catalog cache: saved LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat to cache
SExtractor catalog cache: saved LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.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/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461193.64707691
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_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits exists and is non-empty
Saving wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits to local_wcs_cache/
'wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits' -> 'local_wcs_cache/wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits'
wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits exists and is non-empty
Saving wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits to local_wcs_cache/
'wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits' -> 'local_wcs_cache/wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits'
wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits exists and is non-empty
Saving wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits to local_wcs_cache/
'wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits' -> 'local_wcs_cache/wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits'
wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits exists and is non-empty
Saving wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits to local_wcs_cache/
'wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits' -> 'local_wcs_cache/wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits (1st reference image)
verification OK: wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
Image size: 941.7'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: 11:00:00.428 +30:00:07.99 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_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits (1st new image)
verification OK: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:59:59.468 +30:00:05.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:00:00.428 +30:00:07.99
Second-epoch image center 10:59:59.468 +30:00:05.84
Angular distance between the image centers 0.0035 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits (2nd new image)
verification OK: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:59:59.213 +30:00:00.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:00:00.428 +30:00:07.99
Second-epoch image center 10:59:59.213 +30:00:00.28
Angular distance between the image centers 0.0049 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 10:59:59.468 +30:00:05.84
Second-epoch second image center 10:59:59.213 +30:00:00.28
Angular distance between the image centers 0.00180 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits &> /tmp/tmp.Gmgsz4r2hH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits &> /tmp/tmp.MYE6hEWnzo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits &> /tmp/tmp.6eMItzEdoo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits &> /tmp/tmp.rXUdgOWbYY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
Calibrating the magnitude scale
Found non-empty wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.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_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits and wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits and wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat
Found non-empty wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits and wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat
The reference image (wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits) and catalog (wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat) found
'wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat' -> 'wcsmag.cat'
Read 6277 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.3267 to 174.2388 deg, Dec +24.1798 to +35.3464 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 155.3267 to 174.2388 deg, Dec 24.1798 to 35.3464 deg
Loaded 4197 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): 3040 out of 3199 total matches.
Matched with Tycho-2 3199 out of 6277 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.918250
a=0.000000 b=1.000000 c=22.918250
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6277 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.3267 to 174.2388 deg, Dec +24.1798 to +35.3464 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 155.3267 to 174.2388 deg, Dec 24.1798 to 35.3464 deg
Loaded 4197 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): 3040 out of 3199 total matches.
Matched with Tycho-2 3199 out of 6277 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits:
Forced-photometry filter: calibrated wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits -> calib.txt_param_ref_wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits (aperture=6.3)
Read 6257 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.3266 to 174.2863 deg, Dec +24.1798 to +35.3468 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 155.3266 to 174.2863 deg, Dec 24.1798 to 35.3468 deg
Loaded 4207 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): 3048 out of 3197 total matches.
Matched with Tycho-2 3197 out of 6257 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits:
Forced-photometry filter: calibrated wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits -> calib.txt_param_ref_wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
2.2 pix LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
2.4 pix fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
2.4 pix fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
2.2 pix wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
2.2 pix wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
Limiting magnitude estimates:
15.5 mag. LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
15.5 mag. LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
13.3 mag. fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
13.3 mag. fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 10.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Gmgsz4r2hH (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits' -> 'wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
WCS_IMAGE_NAME=wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
WCS-calibrated image found: wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
Checking if the catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits alredy exist and is non-empty...
Catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
WCS catalog name: wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=426, passed=6277
Got 6277 stars (including 5840 good ones) from the SExtractor catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat
util/solve_plate_with_UCAC5 got 6277 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6219 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6219 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6219 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits N_match=958 sigma_overall_arcsec=0.429 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.412 sigma_q3_arcsec=0.440 sigma_q4_arcsec=0.358 n_q1=235 n_q2=232 n_q3=270 n_q4=221 worst_quadrant_to_overall_ratio=1.245
The image catalog is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits -region wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MYE6hEWnzo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits' -> 'wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
WCS_IMAGE_NAME=wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
WCS-calibrated image found: wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
Checking if the catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits alredy exist and is non-empty...
Catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
WCS catalog name: wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=417, passed=6257
Got 6257 stars (including 5831 good ones) from the SExtractor catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat
util/solve_plate_with_UCAC5 got 6257 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 6197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 6200 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 6200 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits N_match=961 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.423 sigma_q2_arcsec=0.386 sigma_q3_arcsec=0.407 sigma_q4_arcsec=0.320 n_q1=232 n_q2=234 n_q3=274 n_q4=221 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits -region wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6eMItzEdoo (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_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.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_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
WCS_IMAGE_NAME=wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
WCS-calibrated image found: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
Checking if the catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits alredy exist and is non-empty...
Catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
WCS catalog name: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=98, passed=1839
Got 1839 stars (including 1740 good ones) from the SExtractor catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat
util/solve_plate_with_UCAC5 got 1839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 1827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 1827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 1827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 950 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits N_match=950 sigma_overall_arcsec=0.437 sigma_q1_arcsec=0.345 sigma_q2_arcsec=0.538 sigma_q3_arcsec=0.424 sigma_q4_arcsec=0.416 n_q1=208 n_q2=238 n_q3=269 n_q4=235 worst_quadrant_to_overall_ratio=1.232
The image catalog is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits -region wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rXUdgOWbYY (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_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.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_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
WCS_IMAGE_NAME=wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
WCS-calibrated image found: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
Checking if the catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits alredy exist and is non-empty...
Catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
WCS catalog name: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=92, passed=1813
Got 1813 stars (including 1720 good ones) from the SExtractor catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat
util/solve_plate_with_UCAC5 got 1813 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 1803 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 1803 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 1803 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits N_match=949 sigma_overall_arcsec=0.428 sigma_q1_arcsec=0.371 sigma_q2_arcsec=0.530 sigma_q3_arcsec=0.392 sigma_q4_arcsec=0.454 n_q1=213 n_q2=228 n_q3=259 n_q4=249 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits -region wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits sigma_overall=0.429 worst_q_ratio=1.245
ref2=LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits sigma_overall=0.379 worst_q_ratio=1.117
new1=fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits sigma_overall=0.437 worst_q_ratio=1.232
new2=fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits sigma_overall=0.428 worst_q_ratio=1.241
reference average sigma_overall=0.404 worst_q_ratio=1.181
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335_astrometric_residuals.png (958 matched stars from wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336_astrometric_residuals.png (961 matched stars from wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055_astrometric_residuals.png (950 matched stars from wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056_astrometric_residuals.png (949 matched stars from wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits'
Saving fully-calibrated image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits'
Preparing the HTML report for the field LMi-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field LMi-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
SExtractor catalog cache: saved LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat to cache
SExtractor catalog cache: saved LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
Creating symlink local_wcs_cache/wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
Creating symlink local_wcs_cache/wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
Creating symlink local_wcs_cache/wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits exists and is non-empty
wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits exists and is non-empty
wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits exists and is non-empty
wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits (1st reference image)
verification OK: wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
Image size: 941.7'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: 11:00:00.428 +30:00:07.99 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_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits (1st new image)
verification OK: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:59:59.468 +30:00:05.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:00:00.428 +30:00:07.99
Second-epoch image center 10:59:59.468 +30:00:05.84
Angular distance between the image centers 0.0035 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits (2nd new image)
verification OK: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:59:59.213 +30:00:00.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:00:00.428 +30:00:07.99
Second-epoch image center 10:59:59.213 +30:00:00.28
Angular distance between the image centers 0.0049 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 10:59:59.468 +30:00:05.84
Second-epoch second image center 10:59:59.213 +30:00:00.28
Angular distance between the image centers 0.00180 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits &> /tmp/tmp.xMV47Axg0U
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits &> /tmp/tmp.dBQWMnphtv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits &> /tmp/tmp.WA3iOmKZtF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits &> /tmp/tmp.z7wHx29AVA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
Calibrating the magnitude scale
Found non-empty wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.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_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits and wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits and wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat
Found non-empty wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits and wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat
The reference image (wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits) and catalog (wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat) found
'wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat' -> 'wcsmag.cat'
Read 31758 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.1987 to 174.3209 deg, Dec +24.1798 to +35.3640 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 155.1987 to 174.3209 deg, Dec 24.1798 to 35.3640 deg
Loaded 4256 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): 2918 out of 3226 total matches.
Matched with Tycho-2 3226 out of 31758 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.811550
a=0.000000 b=1.000000 c=22.811550
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31758 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.1987 to 174.3209 deg, Dec +24.1798 to +35.3640 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 155.1987 to 174.3209 deg, Dec 24.1798 to 35.3640 deg
Loaded 4256 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): 2918 out of 3226 total matches.
Matched with Tycho-2 3226 out of 31758 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits:
Forced-photometry filter: calibrated wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits -> calib.txt_param_ref_wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits (aperture=5.0)
Read 31789 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.2201 to 174.3325 deg, Dec +24.1798 to +35.3641 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 155.2201 to 174.3325 deg, Dec 24.1798 to 35.3641 deg
Loaded 4254 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): 2901 out of 3226 total matches.
Matched with Tycho-2 3226 out of 31789 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits:
Forced-photometry filter: calibrated wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits -> calib.txt_param_ref_wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
2.1 pix LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
2.2 pix fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
2.2 pix fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
2.0 pix wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
2.1 pix wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
Limiting magnitude estimates:
15.6 mag. LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
15.6 mag. LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
13.7 mag. fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
13.7 mag. fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xMV47Axg0U (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits' -> 'wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
WCS_IMAGE_NAME=wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
WCS-calibrated image found: wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
Checking if the catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits alredy exist and is non-empty...
Catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits
WCS catalog name: wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=1326, passed=31731
Got 31731 stars (including 30344 good ones) from the SExtractor catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat
util/solve_plate_with_UCAC5 got 31731 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 31442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 31442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 31442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits N_match=958 sigma_overall_arcsec=0.414 sigma_q1_arcsec=0.528 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.424 sigma_q4_arcsec=0.337 n_q1=235 n_q2=227 n_q3=271 n_q4=225 worst_quadrant_to_overall_ratio=1.275
The image catalog is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits -region wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dBQWMnphtv (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits' -> 'wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
WCS_IMAGE_NAME=wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
WCS-calibrated image found: wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
Checking if the catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits alredy exist and is non-empty...
Catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits
WCS catalog name: wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=1398, passed=31766
Got 31766 stars (including 30306 good ones) from the SExtractor catalog wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat
util/solve_plate_with_UCAC5 got 31766 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 31541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 31540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 31540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits N_match=959 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.421 sigma_q2_arcsec=0.350 sigma_q3_arcsec=0.448 sigma_q4_arcsec=0.320 n_q1=238 n_q2=231 n_q3=265 n_q4=225 worst_quadrant_to_overall_ratio=1.172
The image catalog is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits -region wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WA3iOmKZtF (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_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.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_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
WCS_IMAGE_NAME=wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
WCS-calibrated image found: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
Checking if the catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits alredy exist and is non-empty...
Catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
WCS catalog name: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=292, passed=12030
Got 12030 stars (including 11722 good ones) from the SExtractor catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat
util/solve_plate_with_UCAC5 got 12030 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 11947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 11946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 11946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits N_match=948 sigma_overall_arcsec=0.420 sigma_q1_arcsec=0.358 sigma_q2_arcsec=0.509 sigma_q3_arcsec=0.418 sigma_q4_arcsec=0.421 n_q1=213 n_q2=237 n_q3=262 n_q4=236 worst_quadrant_to_overall_ratio=1.211
The image catalog is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits -region wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.z7wHx29AVA (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_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.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_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
WCS_IMAGE_NAME=wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
WCS-calibrated image found: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
Checking if the catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits alredy exist and is non-empty...
Catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
WCS catalog name: wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=280, passed=11729
Got 11729 stars (including 11431 good ones) from the SExtractor catalog wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat
util/solve_plate_with_UCAC5 got 11729 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 11655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 11654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 11654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits N_match=950 sigma_overall_arcsec=0.419 sigma_q1_arcsec=0.379 sigma_q2_arcsec=0.511 sigma_q3_arcsec=0.380 sigma_q4_arcsec=0.437 n_q1=219 n_q2=227 n_q3=257 n_q4=247 worst_quadrant_to_overall_ratio=1.220
The image catalog is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits -region wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.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_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-31-37_20.00sec_4.90C_LIGHT_0055.fits
Saving fully-calibrated image wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.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_2026-06-01_CI_LMi-02-Q2b1x1_224130_TTUQ2b1x1_3948770_plq74xwp/wcs_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056.fits
Preparing the HTML report for the field LMi-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 11:05:47.92 +30:12:48.0: 13.21 +/- 0.02 detection
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 10:47:24.34 +29:57:48.4: 13.15 +/- 0.02 detection
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 10:47:29.22 +34:10:23.2: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 10:47:24.34 +29:57:48.4: 13.23 +/- 0.03 detection
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 11:05:47.92 +30:12:48.0: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry reference-image weighted average: 13.21 +/- 0.01
Forced photometry filter REJECTED candidate at 10:47:24.34 +29:57:48.4: ref_mag=13.19 +/- 0.02 new_mean_mag=13.0999 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:05:47.92 +30:12:48.0: ref_mag=13.21 +/- 0.01 new_mean_mag=13.0985 delta=0.12 (need > 0.90)
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 10:49:09.19 +30:15:19.8: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 10:47:29.22 +34:10:23.2: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 11:08:23.37 +25:51:26.9: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 10:49:09.19 +30:15:19.8: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 11:10:38.17 +30:54:30.4: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-26-15_20.00sec_-15.00C_LIGHT_0335.fits at 11:08:02.11 +29:28:39.5: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 11:08:23.37 +25:51:26.9: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 11:08:02.11 +29:28:39.5: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_LMi-02-Q2b1x1_2026-02-22_01-27-03_20.00sec_-14.90C_LIGHT_0336.fits at 11:10:38.17 +30:54:30.4: 16.27 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out53899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54398.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
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 52245_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 52245_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52369_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 52369_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52420_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 52420_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52456_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 52456_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52537_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 52537_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52647_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 52647_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52794_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 52794_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52900_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 52900_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53189_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53189_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53242_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53242_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53303_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53303_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53340_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53340_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53405_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53405_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53420_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53420_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53436_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53436_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53470_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53470_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
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Considering the candidate 53542_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53542_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53566_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53566_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53601_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53601_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53702_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53702_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
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Considering the candidate 53789_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53789_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53832_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53832_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53872_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53872_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53894_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53894_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53899_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
Preparing report for the candidate 53899_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
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Considering the candidate 53900_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53900_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53910_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53910_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 53911_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53911_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53949_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53949_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53972_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53972_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53976_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 53976_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54030_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54030_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54035_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54035_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 54070_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54070_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54073_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54073_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54117_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54117_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54141_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54141_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54145_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
Preparing report for the candidate 54145_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
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Considering the candidate 54189_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54189_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54203_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54203_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54220_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54220_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54233_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
Preparing report for the candidate 54233_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
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Considering the candidate 54243_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54243_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54288_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54288_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54289_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54289_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54316_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54316_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 54338_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54338_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54363_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54363_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54387_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 54387_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54389_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
Preparing report for the candidate 54389_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
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Considering the candidate 54398_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
Preparing report for the candidate 54398_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
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Considering the candidate 23111_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056
The candidate 23111_fd_LMi-02-Q2b1x1_2026-06-01_22-32-14_20.00sec_5.00C_LIGHT_0056 did not pass the final checks
