This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 27.4598 2461248.9598 10.96 21:53:46.01 -12:17:56.8
43.58528 -45.90779 galactic Cap Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.354 Eleonora 0 -0 1 10.8 -0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 21:53:46.01 -12:17:56.8: 15.07 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 21:53:46.01 -12:17:56.8: 15.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 27.4598* 21 53 46.01 -12 17 56.8 11.0 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.9598,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4598 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.4598 2461248.9598 11.48 22:26:08.54 -12:39:31.9
48.71970 -53.08656 galactic Aqr Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.100 Hekate 0 -1 1 11.6 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:26:08.54 -12:39:31.9: 15.27 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:26:08.54 -12:39:31.9: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.9598,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4598 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.4598 2461248.9598 13.13 22:48:04.73 -08:36:23.5
59.54062 -55.46498 galactic Aqr Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.78 Diana -0 -0 1 13.3 -0 -0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:48:04.73 -08:36:23.5: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:48:04.73 -08:36:23.5: 15.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.9598,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4598 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.4598 2461248.9598 13.62 22:23:16.59 -10:26:18.9
51.29973 -51.37582 galactic Aqr Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.736 Harvard -1 -0 1 13.4 0 0
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:23:16.59 -10:26:18.9: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:23:16.59 -10:26:18.9: 15.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461248.9598,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.4598 13.62CV 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: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
First image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Last image: 2461248.96015111 27.07.2026 11:02:27.056 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.00
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: 7 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): 5374
Objects passed selection criteria: 5363
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 4650
Average stars matched: 3837.5 (82.5269 %)
Memory usage VmPeak: 232776 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 27 08:04:40 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: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
First image: 2461211.88265034 20.06.2026 09:10:50.989 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Last image: 2461248.96015111 27.07.2026 11:02:27.056 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
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: 21 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): 31888
Objects passed selection criteria: 31804
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 28510.2
Average stars matched: 25263.2 (88.6111 %)
Memory usage VmPeak: 257576 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 27 08:09:09 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.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: 2461248.95951456
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_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits exists and is non-empty
Saving wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits to local_wcs_cache/
'wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits'
wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits exists and is non-empty
Saving wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits to local_wcs_cache/
'wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits'
wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits'
wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits (1st reference image)
verification OK: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Image size: 937.3'x624.3' 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: 22:17:07.716 -09:59:55.69 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:13.560 -10:04:57.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:13.560 -10:04:57.16
Angular distance between the image centers 0.0871 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:10.846 -10:05:13.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:10.846 -10:05:13.38
Angular distance between the image centers 0.0892 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 22:17:13.560 -10:04:57.16
Second-epoch second image center 22:17:10.846 -10:05:13.38
Angular distance between the image centers 0.01201 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits &> /tmp/tmp.cOAdRNWmOz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits &> /tmp/tmp.HY9az7Tstg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits &> /tmp/tmp.MY5QIJHRKI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits &> /tmp/tmp.Y0rgzGZppQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.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_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
Found non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
The reference image (wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits) and catalog (wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat) found
'wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat' -> 'wcsmag.cat'
Read 5318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 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 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Loaded 5068 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): 3783 out of 3855 total matches.
Matched with Tycho-2 3855 out of 5318 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.580000
a=0.000000 b=1.000000 c=22.580000
From vast_summary.log: estimated ref. image limiting mag.: -8.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 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 326.2566 to 342.3670 deg, Dec -15.2671 to -4.6696 deg
Loaded 5068 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): 3783 out of 3855 total matches.
Matched with Tycho-2 3855 out of 5318 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits (aperture=6.4)
Read 8439 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4086 deg, Dec -15.2463 to -4.6697 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 326.2518 to 342.4086 deg, Dec -15.2463 to -4.6697 deg
Loaded 5075 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): 4285 out of 4418 total matches.
Matched with Tycho-2 4418 out of 8439 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
2.4 pix Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
2.1 pix fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
2.1 pix fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
2.3 pix wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
2.4 pix wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Limiting magnitude estimates:
14.6 mag. Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
15.2 mag. Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
13.9 mag. fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
13.8 mag. fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
All-image limiting magnitude estimate: 13.8 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.cOAdRNWmOz (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/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.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_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=331, bad_region=0, passed=5318
Got 5318 stars (including 4983 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
util/solve_plate_with_UCAC5 got 5318 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 890 matched stars entering correct_measured_positions(), 880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 890 matched stars entering correct_measured_positions(), 5253 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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 890 matched stars entering correct_measured_positions(), 5249 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 890 matched stars entering correct_measured_positions(), 5249 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 890 stars left (next iteration limit 979)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits N_match=890 sigma_overall_arcsec=0.447 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.512 sigma_q3_arcsec=0.399 sigma_q4_arcsec=0.589 n_q1=245 n_q2=217 n_q3=218 n_q4=210 worst_quadrant_to_overall_ratio=1.317
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits -region wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.HY9az7Tstg (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/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.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_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits 856.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits'
This WCS solution (swarp) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=484, bad_region=0, passed=8439
Got 8439 stars (including 7944 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 8439 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 8340 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 8341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 8341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 901 stars left (next iteration limit 991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits (swarp) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits N_match=901 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.274 sigma_q2_arcsec=0.411 sigma_q3_arcsec=0.345 sigma_q4_arcsec=0.440 n_q1=245 n_q2=211 n_q3=225 n_q4=220 worst_quadrant_to_overall_ratio=1.222
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits -region wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MY5QIJHRKI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=453, bad_region=0, passed=2665
Got 2665 stars (including 2211 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat
util/solve_plate_with_UCAC5 got 2665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.4)
Done reading UCAC5 zone files...
Matched 889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 2610 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.4)
Done reading UCAC5 zone files...
Matched 888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 2609 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 2609 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 887 stars left (next iteration limit 975)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=887 robust_rms=12.817 arcsec
SIP_REFIT: SIP order 3 trial: matched=887 robust_rms=0.490 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=887 robust_rms_before=0.932 arcsec robust_rms_before_corrected=0.328 arcsec robust_rms_after=0.490 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.328 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits N_match=887 sigma_overall_arcsec=0.348 sigma_q1_arcsec=0.375 sigma_q2_arcsec=0.398 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.317 n_q1=200 n_q2=235 n_q3=208 n_q4=244 worst_quadrant_to_overall_ratio=1.144
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Y0rgzGZppQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=329, bad_region=0, passed=2368
Got 2368 stars (including 2038 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat
util/solve_plate_with_UCAC5 got 2368 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.4)
Done reading UCAC5 zone files...
Matched 894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 2335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.4)
Done reading UCAC5 zone files...
Matched 893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 2334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 2334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 892 stars left (next iteration limit 981)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=892 robust_rms=12.770 arcsec
SIP_REFIT: SIP order 3 trial: matched=892 robust_rms=0.500 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=892 robust_rms_before=0.944 arcsec robust_rms_before_corrected=0.321 arcsec robust_rms_after=0.500 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.321 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits N_match=892 sigma_overall_arcsec=0.337 sigma_q1_arcsec=0.356 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.327 sigma_q4_arcsec=0.306 n_q1=202 n_q2=234 n_q3=212 n_q4=244 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits sigma_overall=0.447 worst_q_ratio=1.317
ref2=Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits sigma_overall=0.360 worst_q_ratio=1.222
new1=fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits sigma_overall=0.348 worst_q_ratio=1.144
new2=fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits sigma_overall=0.337 worst_q_ratio=1.108
reference average sigma_overall=0.4035 worst_q_ratio=1.2695
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1_astrometric_residuals.png (890 matched stars from wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2_astrometric_residuals.png (901 matched stars from wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372_astrometric_residuals.png (887 matched stars from wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373_astrometric_residuals.png (892 matched stars from wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits'
Preparing the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 21:53:46.01 -12:17:56.8: 15.07 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 21:53:46.01 -12:17:56.8: 15.67 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out23188.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23188_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 23188_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00456_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 00456_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 22:19:54.42 -14:24:07.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 12s
Prepared the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:53:46.01 -12:17:56.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.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_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits exists and is non-empty
wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits exists and is non-empty
wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits (1st reference image)
verification OK: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Image size: 937.3'x624.3' 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: 22:17:07.716 -09:59:55.69 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:13.560 -10:04:57.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:13.560 -10:04:57.16
Angular distance between the image centers 0.0871 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:10.846 -10:05:13.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:07.716 -09:59:55.69
Second-epoch image center 22:17:10.846 -10:05:13.38
Angular distance between the image centers 0.0892 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 22:17:13.560 -10:04:57.16
Second-epoch second image center 22:17:10.846 -10:05:13.38
Angular distance between the image centers 0.01201 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits &> /tmp/tmp.x236SvuPa8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits &> /tmp/tmp.BFG8W8yDSt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits &> /tmp/tmp.dTzLLXy5Qi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits &> /tmp/tmp.PpWPAn3oXB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.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_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
Found non-empty wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits and wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
The reference image (wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits) and catalog (wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat) found
'wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat' -> 'wcsmag.cat'
Read 31665 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 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 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Loaded 5086 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): 4178 out of 4455 total matches.
Matched with Tycho-2 4455 out of 31665 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.443700
a=0.000000 b=1.000000 c=22.443700
From vast_summary.log: estimated ref. image limiting mag.: -7.72
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.72
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.72
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31665 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 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 326.2518 to 342.4049 deg, Dec -15.2687 to -4.6696 deg
Loaded 5086 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): 4178 out of 4455 total matches.
Matched with Tycho-2 4455 out of 31665 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits (aperture=5.0)
Read 43541 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2516 to 342.4086 deg, Dec -15.2553 to -4.6543 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 326.2516 to 342.4086 deg, Dec -15.2553 to -4.6543 deg
Loaded 5090 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): 4047 out of 4457 total matches.
Matched with Tycho-2 4457 out of 43541 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits -> calib.txt_param_ref_wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 18 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
2.3 pix Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
1.9 pix fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
1.9 pix fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
2.2 pix wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
2.3 pix wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Limiting magnitude estimates:
14.7 mag. Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
15.3 mag. Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
14.0 mag. fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
13.9 mag. fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
All-image limiting magnitude estimate: 13.9 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.x236SvuPa8 (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/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.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_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1237, bad_region=0, passed=31646
Got 31646 stars (including 30372 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat
util/solve_plate_with_UCAC5 got 31646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 31229 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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 31229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 31229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 880 stars left (next iteration limit 968)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits N_match=880 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.564 sigma_q3_arcsec=0.419 sigma_q4_arcsec=0.595 n_q1=248 n_q2=201 n_q3=221 n_q4=210 worst_quadrant_to_overall_ratio=1.298
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits -region wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BFG8W8yDSt (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/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.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_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits 856.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits' -> 'wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits'
This WCS solution (swarp) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS-calibrated image found: wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
Checking if the catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat corresponding to the image wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits
WCS catalog name: wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=39, blended=2096, bad_region=0, passed=43502
Got 43502 stars (including 41351 good ones) from the SExtractor catalog wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat
util/solve_plate_with_UCAC5 got 43502 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 42954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 42954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 42954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 897 stars left (next iteration limit 986)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits N_match=897 sigma_overall_arcsec=0.356 sigma_q1_arcsec=0.261 sigma_q2_arcsec=0.415 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.474 n_q1=246 n_q2=204 n_q3=231 n_q4=216 worst_quadrant_to_overall_ratio=1.334
The image catalog is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits -region wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dTzLLXy5Qi (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=631, bad_region=1, passed=20259
Got 20259 stars (including 19588 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat
util/solve_plate_with_UCAC5 got 20259 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.3)
Done reading UCAC5 zone files...
Matched 882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 19892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 371 to 430 (Dec -15.7 to -4.3)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 19894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 19894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 880 stars left (next iteration limit 968)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits N_match=880 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.372 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.270 n_q1=202 n_q2=232 n_q3=205 n_q4=241 worst_quadrant_to_overall_ratio=1.207
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PpWPAn3oXB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
Checking if the catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
WCS catalog name: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=601, bad_region=1, passed=19399
Got 19399 stars (including 18761 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat
util/solve_plate_with_UCAC5 got 19399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.3)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 19056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 371 to 430 (Dec -15.7 to -4.3)
Done reading UCAC5 zone files...
Matched 880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 19057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 19057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 880 stars left (next iteration limit 966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits N_match=880 sigma_overall_arcsec=0.341 sigma_q1_arcsec=0.355 sigma_q2_arcsec=0.409 sigma_q3_arcsec=0.300 sigma_q4_arcsec=0.330 n_q1=200 n_q2=233 n_q3=207 n_q4=240 worst_quadrant_to_overall_ratio=1.199
The image catalog is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits -region wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-01-32_20.00sec_-0.00C_LIGHTs_0372.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Aqr-04-Q1b1x1_061931_TTUQ1b1x1_2488295_bf0dDofc/wcs_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373.fits
Preparing the HTML report for the field Aqr-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:47:39.40 -11:22:18.0: 13.16 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:41:53.84 -12:24:22.9: 11.09 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:37:00.35 -07:34:42.8: 10.96 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:44:35.89 -06:52:17.9: 12.23 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:21:07.43 -06:25:55.7: 13.39 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 21:54:59.81 -11:58:10.4: 10.58 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:37:17.52 -13:57:08.7: 12.92 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:45:53.17 -06:52:43.2: 12.89 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:17:02.30 -08:06:03.0: 13.84 +/- 0.08 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:44:23.26 -14:42:35.2: 11.31 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:17:02.30 -08:06:03.0: 13.92 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:41:53.84 -12:24:22.9: 11.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:47:39.40 -11:22:18.0: 13.14 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 22:17:02.30 -08:06:03.0: ref_mag=13.90 +/- 0.05 new_mean_mag=13.8729 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 11.08 +/- 0.00
Forced photometry filter REJECTED candidate at 22:41:53.84 -12:24:22.9: ref_mag=11.08 +/- 0.00 new_mean_mag=11.5435 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:44:35.89 -06:52:17.9: 12.20 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:45:53.17 -06:52:43.2: 12.82 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:37:00.35 -07:34:42.8: 10.92 +/- 0.00 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 21:54:59.81 -11:58:10.4: 10.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:37:17.52 -13:57:08.7: 12.79 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:21:07.43 -06:25:55.7: 13.33 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 22:47:39.40 -11:22:18.0: ref_mag=13.14 +/- 0.03 new_mean_mag=13.2848 delta=-0.14 (need > 0.90)
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry reference-image weighted average: 10.92 +/- 0.00
Forced photometry reference-image weighted average: 10.52 +/- 0.00
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter REJECTED candidate at 22:44:35.89 -06:52:17.9: ref_mag=12.21 +/- 0.01 new_mean_mag=12.4860 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:45:53.17 -06:52:43.2: ref_mag=12.84 +/- 0.02 new_mean_mag=12.9884 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Forced photometry filter REJECTED candidate at 22:37:00.35 -07:34:42.8: ref_mag=10.92 +/- 0.00 new_mean_mag=11.1017 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:54:59.81 -11:58:10.4: ref_mag=10.52 +/- 0.00 new_mean_mag=10.8315 delta=-0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:37:17.52 -13:57:08.7: ref_mag=12.82 +/- 0.02 new_mean_mag=13.0275 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:21:07.43 -06:25:55.7: ref_mag=13.34 +/- 0.03 new_mean_mag=13.6727 delta=-0.33 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:44:23.26 -14:42:35.2: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.01
Forced photometry filter REJECTED candidate at 22:44:23.26 -14:42:35.2: ref_mag=11.24 +/- 0.01 new_mean_mag=11.1535 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:45:08.19 -06:39:17.7: 12.33 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:48:04.73 -08:36:23.5: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:26:08.54 -12:39:31.9: 15.27 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:39:58.80 -14:33:11.0: 12.61 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-10-50_20.00sec_4.90C_LIGHT_0410_stack1.fits at 22:23:16.59 -10:26:18.9: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:45:08.19 -06:39:17.7: 12.24 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:39:58.80 -14:33:11.0: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Forced photometry filter REJECTED candidate at 22:45:08.19 -06:39:17.7: ref_mag=12.26 +/- 0.01 new_mean_mag=12.4134 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:39:58.80 -14:33:11.0: ref_mag=12.56 +/- 0.02 new_mean_mag=12.4240 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:48:04.73 -08:36:23.5: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:23:16.59 -10:26:18.9: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q1b1x1_2026-06-20_04-11-39_20.00sec_5.00C_LIGHT_0411_stack2.fits at 22:26:08.54 -12:39:31.9: 15.87 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out62278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62768.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 62134_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62134_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62137_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62137_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62141_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62141_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62143_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62143_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62144_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62144_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62146_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62146_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62147_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62147_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62222_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62222_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62223_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62223_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 21:53:46.00 -12:17:56.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 62239_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62239_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62243_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62243_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62278_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 62278_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 62290_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62290_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
**** FOUND 22:43:10.21 -06:58:30.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 62416_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62416_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62421_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 62421_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks
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Considering the candidate 62596_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 62596_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 62768_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
Preparing report for the candidate 62768_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
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Considering the candidate 01862_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373
The candidate 01862_fd_Aqr-04-Q1b1x1_2026-07-27_06-02-27_20.00sec_0.00C_LIGHTs_0373 did not pass the final checks