This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 04.2659 2461256.7659 9.16 20:01:33.00 -05:50:02.7
35.71727 -18.24019 galactic Aql Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.3 Juno 1 -0 1 9.2 -0 -0
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:01:33.00 -05:50:02.7: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:01:33.00 -05:50:02.7: 15.47 +/- 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,2461256.7659,9.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260804.2659 9.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 04.2659 2461256.7659 12.23 19:43:40.82 -04:40:14.5
34.71538 -13.74394 galactic Aql Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.345 Tercidina 0 -1 1 12.4 -0 0
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:43:40.82 -04:40:14.5: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:43:40.82 -04:40:14.5: 15.81 +/- 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,2461256.7659,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260804.2659 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 04.2659 2461256.7659 13.13 19:53:39.49 -06:10:27.7
34.47774 -16.63787 galactic Aql Second-epoch detections are separated by 1.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.313 Chaldaea 0 0 0 13.2 -0 0
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:53:39.49 -06:10:27.7: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:53:39.49 -06:10:27.7: 15.64 +/- 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,2461256.7659,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260804.2659 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 08 04.2659 2461256.7659 13.30 20:06:46.73 -02:43:04.8
39.26022 -17.97670 galactic Aql Second-epoch detections are separated by 0.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.365 Corduba 1 -1 1 13.2 0 0
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:06:46.73 -02:43:04.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:06:46.73 -02:43:04.8: 15.71 +/- 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,2461256.7659,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260804.2659 13.30CV 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: 2461203.88244201 12.06.2026 09:10:32.990 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
First image: 2461203.88244201 12.06.2026 09:10:32.990 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Last image: 2461256.76625598 04.08.2026 06:23:14.517 /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
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: 6 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 13879
Objects passed selection criteria: 13858
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 12583.8
Average stars matched: 12282 (97.6021 %)
Memory usage VmPeak: 240896 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 4 01:38:04 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: 2461203.88244201 12.06.2026 09:10:32.990 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
First image: 2461203.88244201 12.06.2026 09:10:32.990 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Last image: 2461256.76625598 04.08.2026 06:23:14.517 /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 59
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 80 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 127395
Objects passed selection criteria: 127226
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 113000
Average stars matched: 107740 (95.3453 %)
Memory usage VmPeak: 531244 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 4 01:40:23 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.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: 2461256.76550150
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits'
wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits exists and is non-empty
Saving wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits to local_wcs_cache/
'wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits' -> 'local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits'
wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits exists and is non-empty
Saving wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits to local_wcs_cache/
'wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits' -> 'local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits'
wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits exists and is non-empty
Saving wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits to local_wcs_cache/
'wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits' -> 'local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:42:53.275 -01:59:56.67 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_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits (1st new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
Image size: 936.8'x623.9' 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: 19:42:51.675 -01:59:47.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:53.275 -01:59:56.67
Second-epoch image center 19:42:51.675 -01:59:47.90
Angular distance between the image centers 0.0071 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits (2nd new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Image size: 936.8'x623.9' 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: 19:42:48.872 -02:00:06.67 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:42:53.275 -01:59:56.67
Second-epoch image center 19:42:48.872 -02:00:06.67
Angular distance between the image centers 0.0185 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 19:42:51.675 -01:59:47.90
Second-epoch second image center 19:42:48.872 -02:00:06.67
Angular distance between the image centers 0.01278 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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits &> /tmp/tmp.yTtT96NF9p
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits &> /tmp/tmp.KYZdLL8Da1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits &> /tmp/tmp.8AZqzPteMu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits &> /tmp/tmp.oDajHOJ3tc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
The reference image (wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits) and catalog (wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat) found
'wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat' -> 'wcsmag.cat'
Read 20227 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8574 to 303.5971 deg, Dec -7.2599 to +3.2634 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 287.8574 to 303.5971 deg, Dec -7.2599 to 3.2634 deg
Loaded 10289 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): 8488 out of 8950 total matches.
Matched with Tycho-2 8950 out of 20227 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.706950
a=0.000000 b=1.000000 c=22.706950
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.96
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.96
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 20227 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8574 to 303.5971 deg, Dec -7.2599 to +3.2634 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 287.8574 to 303.5971 deg, Dec -7.2599 to 3.2634 deg
Loaded 10289 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): 8488 out of 8950 total matches.
Matched with Tycho-2 8950 out of 20227 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (aperture=6.1)
Read 20355 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8562 to 303.5949 deg, Dec -7.2521 to +3.2742 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 287.8562 to 303.5949 deg, Dec -7.2521 to 3.2742 deg
Loaded 10292 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): 8460 out of 8944 total matches.
Matched with Tycho-2 8944 out of 20355 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
2.3 pix Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
2.9 pix fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
2.8 pix fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Limiting magnitude estimates:
15.0 mag. Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
15.0 mag. Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
14.5 mag. fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
14.5 mag. fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.8 (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.yTtT96NF9p (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits' -> 'wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1243, bad_region=5559, passed=20227
Got 20227 stars (including 13746 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
util/solve_plate_with_UCAC5 got 20227 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 4896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 15889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 15889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 15889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4895 stars left (next iteration limit 5385)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits N_match=4895 sigma_overall_arcsec=0.462 sigma_q1_arcsec=0.391 sigma_q2_arcsec=0.579 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.552 n_q1=1710 n_q2=1061 n_q3=1253 n_q4=871 worst_quadrant_to_overall_ratio=1.253
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits -region wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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.KYZdLL8Da1 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits' -> 'wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.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/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1255, bad_region=5422, passed=20355
Got 20355 stars (including 13974 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat
util/solve_plate_with_UCAC5 got 20355 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 4900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 16095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 16095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 16095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4900 stars left (next iteration limit 5390)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits N_match=4900 sigma_overall_arcsec=0.467 sigma_q1_arcsec=0.407 sigma_q2_arcsec=0.531 sigma_q3_arcsec=0.457 sigma_q4_arcsec=0.521 n_q1=1731 n_q2=1024 n_q3=1295 n_q4=850 worst_quadrant_to_overall_ratio=1.138
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits -region wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.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.8AZqzPteMu (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=707, bad_region=2856, passed=13434
Got 13434 stars (including 10086 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat
util/solve_plate_with_UCAC5 got 13434 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 4893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 11209 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 11209 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 11209 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 4893 stars left (next iteration limit 5382)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4893 robust_rms=6.923 arcsec worst_quadrant_rms=8.971 arcsec
SIP_REFIT: SIP order 3 trial: matched=4893 robust_rms=0.584 arcsec worst_quadrant_rms=0.723 arcsec
SIP_REFIT: SIP order 5 trial: matched=4893 robust_rms=0.562 arcsec worst_quadrant_rms=0.705 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4893 robust_rms_before=0.776 arcsec robust_rms_before_corrected=0.596 arcsec robust_rms_after=0.584 arcsec worst_quadrant_rms_before=0.780 worst_quadrant_rms_after=0.723
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.780 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits N_match=4893 sigma_overall_arcsec=0.533 sigma_q1_arcsec=0.444 sigma_q2_arcsec=0.698 sigma_q3_arcsec=0.489 sigma_q4_arcsec=0.677 n_q1=1787 n_q2=979 n_q3=1320 n_q4=807 worst_quadrant_to_overall_ratio=1.309
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits -region wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.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.oDajHOJ3tc (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=710, bad_region=2893, passed=13396
Got 13396 stars (including 10020 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat
util/solve_plate_with_UCAC5 got 13396 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 4890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 11152 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 11152 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 11152 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 4892 stars left (next iteration limit 5379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4892 robust_rms=6.914 arcsec worst_quadrant_rms=9.002 arcsec
SIP_REFIT: SIP order 3 trial: matched=4892 robust_rms=0.574 arcsec worst_quadrant_rms=0.729 arcsec
SIP_REFIT: SIP order 5 trial: matched=4892 robust_rms=0.557 arcsec worst_quadrant_rms=0.690 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4892 robust_rms_before=0.763 arcsec robust_rms_before_corrected=0.590 arcsec robust_rms_after=0.557 arcsec worst_quadrant_rms_before=0.783 worst_quadrant_rms_after=0.690
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Image size: 937.3'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:42:48.878 -02:00:06.89 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 13396 stars ###
'wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/correct_sextractor_wcs_catalog_usingxy2sky1500431.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.763 -> 0.557 arcsec)
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits N_match=4892 sigma_overall_arcsec=0.556 sigma_q1_arcsec=0.468 sigma_q2_arcsec=0.719 sigma_q3_arcsec=0.524 sigma_q4_arcsec=0.658 n_q1=1786 n_q2=982 n_q3=1319 n_q4=805 worst_quadrant_to_overall_ratio=1.294
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits -region wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.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=Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits sigma_overall=0.462 worst_q_ratio=1.253
ref2=Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits sigma_overall=0.467 worst_q_ratio=1.138
new1=fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits sigma_overall=0.533 worst_q_ratio=1.309
new2=fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits sigma_overall=0.556 worst_q_ratio=1.294
reference average sigma_overall=0.4645 worst_q_ratio=1.1955
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226_astrometric_residuals.png (4895 matched stars from wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290_astrometric_residuals.png (4900 matched stars from wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250_astrometric_residuals.png (4893 matched stars from wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251_astrometric_residuals.png (4892 matched stars from wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits'
Saving fully-calibrated image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits'
Preparing the HTML report for the field Aql-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:07:22.09 +01:38:03.1: 12.07 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:01:33.00 -05:50:02.7: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:01:33.00 -05:50:02.7: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:07:22.09 +01:38:03.1: 12.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter REJECTED candidate at 20:07:22.09 +01:38:03.1: ref_mag=12.07 +/- 0.01 new_mean_mag=12.0617 delta=0.00 (need > 0.90)
Adding exclusion_list_local.txt__out31156.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31156_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
Preparing report for the candidate 31156_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31164_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 31164_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 19:30:47.71 -02:47:44.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31170_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 31170_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30369_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 30369_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 19:40:57.97 -03:30:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30130_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 30130_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 20:01:47.04 +02:07:20.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Aql-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:01:33.00 -05:50:02.7
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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.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_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits exists and is non-empty
wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits exists and is non-empty
wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits exists and is non-empty
wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:42:53.275 -01:59:56.67 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_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits (1st new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
Image size: 936.8'x623.9' 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: 19:42:51.675 -01:59:47.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:53.275 -01:59:56.67
Second-epoch image center 19:42:51.675 -01:59:47.90
Angular distance between the image centers 0.0071 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits (2nd new image)
verification OK: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Image size: 936.8'x623.9' 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: 19:42:48.872 -02:00:06.67 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:42:53.275 -01:59:56.67
Second-epoch image center 19:42:48.872 -02:00:06.67
Angular distance between the image centers 0.0185 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 19:42:51.675 -01:59:47.90
Second-epoch second image center 19:42:48.872 -02:00:06.67
Angular distance between the image centers 0.01278 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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits &> /tmp/tmp.OjsFR5SWn7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits &> /tmp/tmp.JFoA6X8jmO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits &> /tmp/tmp.3MexBtiXKe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits &> /tmp/tmp.pOJ6RPSuZw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
Found non-empty wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits and wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
The reference image (wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits) and catalog (wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat) found
'wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat' -> 'wcsmag.cat'
Read 167162 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8558 to 303.5989 deg, Dec -7.2624 to +3.2650 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 287.8558 to 303.5989 deg, Dec -7.2624 to 3.2650 deg
Loaded 10296 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): 7300 out of 9230 total matches.
Matched with Tycho-2 9230 out of 167162 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.545200
a=0.000000 b=1.000000 c=22.545200
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.14
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.14
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 167162 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8558 to 303.5989 deg, Dec -7.2624 to +3.2650 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 287.8558 to 303.5989 deg, Dec -7.2624 to 3.2650 deg
Loaded 10296 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): 7300 out of 9230 total matches.
Matched with Tycho-2 9230 out of 167162 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits (aperture=4.7)
Read 183128 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.8553 to 303.5977 deg, Dec -7.2536 to +3.2758 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 287.8553 to 303.5977 deg, Dec -7.2536 to 3.2758 deg
Loaded 10297 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): 7125 out of 9225 total matches.
Matched with Tycho-2 9225 out of 183128 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Forced-photometry filter: calibrated wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits -> calib.txt_param_ref_wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 45 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
2.1 pix Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
2.7 pix fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
2.6 pix fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Limiting magnitude estimates:
15.1 mag. Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
15.2 mag. Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
14.6 mag. fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
14.6 mag. fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 13.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OjsFR5SWn7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits' -> 'wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=19123, bad_region=31897, passed=167147
Got 167147 stars (including 120817 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat
util/solve_plate_with_UCAC5 got 167147 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 143311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 143311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 143313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 4912 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits N_match=4912 sigma_overall_arcsec=0.454 sigma_q1_arcsec=0.384 sigma_q2_arcsec=0.547 sigma_q3_arcsec=0.433 sigma_q4_arcsec=0.538 n_q1=1725 n_q2=1034 n_q3=1334 n_q4=819 worst_quadrant_to_overall_ratio=1.205
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits -region wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.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.JFoA6X8jmO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits' -> 'wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.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/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS_IMAGE_NAME=wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS-calibrated image found: wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
Checking if the catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits alredy exist and is non-empty...
Catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat corresponding to the image wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits
WCS catalog name: wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=21567, bad_region=35769, passed=183109
Got 183109 stars (including 130765 good ones) from the SExtractor catalog wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat
util/solve_plate_with_UCAC5 got 183109 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 4915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 156363 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 156363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 156363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4916 stars left (next iteration limit 5406)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits N_match=4916 sigma_overall_arcsec=0.443 sigma_q1_arcsec=0.399 sigma_q2_arcsec=0.510 sigma_q3_arcsec=0.423 sigma_q4_arcsec=0.501 n_q1=1717 n_q2=991 n_q3=1376 n_q4=832 worst_quadrant_to_overall_ratio=1.150
The image catalog is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits -region wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.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.3MexBtiXKe (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=10260, bad_region=19247, passed=104545
Got 104545 stars (including 78398 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat
util/solve_plate_with_UCAC5 got 104545 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 4905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 90050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 90050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 90050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 4904 stars left (next iteration limit 5394)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits N_match=4904 sigma_overall_arcsec=0.522 sigma_q1_arcsec=0.453 sigma_q2_arcsec=0.687 sigma_q3_arcsec=0.487 sigma_q4_arcsec=0.644 n_q1=1822 n_q2=914 n_q3=1394 n_q4=774 worst_quadrant_to_overall_ratio=1.316
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits -region wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.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.pOJ6RPSuZw (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
WCS_IMAGE_NAME=wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
WCS-calibrated image found: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Checking if the catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat corresponding to the image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
WCS catalog name: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=10647, bad_region=19677, passed=106769
Got 106769 stars (including 80041 good ones) from the SExtractor catalog wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat
util/solve_plate_with_UCAC5 got 106769 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 4902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 91889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 91889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 91888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 4902 stars left (next iteration limit 5392)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits N_match=4902 sigma_overall_arcsec=0.535 sigma_q1_arcsec=0.450 sigma_q2_arcsec=0.697 sigma_q3_arcsec=0.518 sigma_q4_arcsec=0.663 n_q1=1823 n_q2=912 n_q3=1395 n_q4=772 worst_quadrant_to_overall_ratio=1.303
The image catalog is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits -region wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.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_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-22-09_20.00sec_-0.00C_LIGHT_0250.fits
Saving fully-calibrated image wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-04_CI_Aql-04-Q2b1x1_013526_TTUQ2b1x1_1474522_7ROdmgd3/wcs_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251.fits
Preparing the HTML report for the field Aql-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:39:09.38 +01:51:00.9: 14.11 +/- 0.08 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:29:09.96 -04:45:14.0: 13.87 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:53:07.01 -03:11:58.1: 13.87 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:53:17.77 +00:51:22.5: 13.61 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:40:13.72 -05:06:21.6: 13.69 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:37:41.96 +01:57:52.7: 13.68 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:58:44.58 -01:02:04.2: 13.59 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:52:31.15 -02:32:16.1: 14.75 +/- 0.14 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:37:02.49 +00:43:21.1: 13.67 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:03:31.09 -00:22:32.3: 13.56 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:29:09.96 -04:45:14.0: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:53:07.01 -03:11:58.1: 14.01 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 19:29:09.96 -04:45:14.0: ref_mag=13.94 +/- 0.05 new_mean_mag=13.8455 delta=0.10 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:52:31.15 -02:32:16.1: 14.38 +/- 0.09 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:53:17.77 +00:51:22.5: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:37:02.49 +00:43:21.1: 14.06 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:39:09.38 +01:51:00.9: 13.94 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:37:41.96 +01:57:52.7: 13.86 +/- 0.06 detection
Forced photometry filter REJECTED candidate at 19:53:07.01 -03:11:58.1: ref_mag=13.94 +/- 0.05 new_mean_mag=14.0101 delta=-0.07 (need > 0.90)
Forced photometry reference-image weighted average: 14.49 +/- 0.08
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Forced photometry filter REJECTED candidate at 19:52:31.15 -02:32:16.1: ref_mag=14.49 +/- 0.08 new_mean_mag=14.3201 delta=0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:53:17.77 +00:51:22.5: ref_mag=13.63 +/- 0.04 new_mean_mag=13.7591 delta=-0.13 (need > 0.90)
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:40:13.72 -05:06:21.6: 13.67 +/- 0.05 detection
Forced photometry filter REJECTED candidate at 19:37:02.49 +00:43:21.1: ref_mag=13.81 +/- 0.04 new_mean_mag=13.6990 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter REJECTED candidate at 19:37:41.96 +01:57:52.7: ref_mag=13.76 +/- 0.04 new_mean_mag=13.9384 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:39:09.38 +01:51:00.9: ref_mag=14.00 +/- 0.05 new_mean_mag=13.9861 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter REJECTED candidate at 19:40:13.72 -05:06:21.6: ref_mag=13.68 +/- 0.04 new_mean_mag=13.7178 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:58:44.58 -01:02:04.2: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry filter REJECTED candidate at 19:58:44.58 -01:02:04.2: ref_mag=13.53 +/- 0.04 new_mean_mag=13.7673 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:03:31.09 -00:22:32.3: 13.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter REJECTED candidate at 20:03:31.09 -00:22:32.3: ref_mag=13.51 +/- 0.03 new_mean_mag=13.7561 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:47:23.92 +00:27:57.0: 13.29 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:53:39.49 -06:10:27.7: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:04:38.87 +01:09:22.1: 13.22 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:48:37.07 +00:17:01.9: 12.89 +/- 0.03 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:43:40.82 -04:40:14.5: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:49:37.20 -04:32:44.3: 13.43 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:53:39.49 -06:10:27.7: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:48:37.07 +00:17:01.9: 12.89 +/- 0.02 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:47:23.92 +00:27:57.0: 13.36 +/- 0.04 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:04:38.87 +01:09:22.1: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter REJECTED candidate at 19:48:37.07 +00:17:01.9: ref_mag=12.89 +/- 0.02 new_mean_mag=13.0480 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:47:23.92 +00:27:57.0: ref_mag=13.32 +/- 0.03 new_mean_mag=13.3422 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Forced photometry filter REJECTED candidate at 20:04:38.87 +01:09:22.1: ref_mag=13.17 +/- 0.03 new_mean_mag=13.2024 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:06:46.73 -02:43:04.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:43:40.82 -04:40:14.5: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:02:11.07 -05:18:03.8: 13.34 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:49:12.74 +00:00:46.1: 13.53 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:49:37.20 -04:32:44.3: 13.35 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter REJECTED candidate at 19:49:37.20 -04:32:44.3: ref_mag=13.39 +/- 0.03 new_mean_mag=13.2223 delta=0.16 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:06:46.73 -02:43:04.8: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:49:12.74 +00:00:46.1: 13.50 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:02:11.07 -05:18:03.8: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Forced photometry filter REJECTED candidate at 19:49:12.74 +00:00:46.1: ref_mag=13.52 +/- 0.04 new_mean_mag=13.5378 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter REJECTED candidate at 20:02:11.07 -05:18:03.8: ref_mag=13.33 +/- 0.03 new_mean_mag=13.4736 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:47:38.79 -01:54:00.2: 13.55 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:55:52.79 -00:44:59.7: 13.63 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:47:38.79 -01:54:00.2: 13.58 +/- 0.05 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:47:46.26 -00:04:17.5: 13.84 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter REJECTED candidate at 19:47:38.79 -01:54:00.2: ref_mag=13.57 +/- 0.03 new_mean_mag=13.5301 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:53:57.16 +00:33:33.9: 13.74 +/- 0.06 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:55:52.79 -00:44:59.7: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry filter REJECTED candidate at 19:55:52.79 -00:44:59.7: ref_mag=13.51 +/- 0.04 new_mean_mag=13.6113 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:47:46.26 -00:04:17.5: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:29:20.59 -01:24:12.6: 13.71 +/- 0.08 detection
Forced photometry filter REJECTED candidate at 19:47:46.26 -00:04:17.5: ref_mag=13.79 +/- 0.05 new_mean_mag=13.7632 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 20:06:13.32 -04:10:29.5: 13.80 +/- 0.07 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:53:57.16 +00:33:33.9: 13.78 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.05
Forced photometry filter REJECTED candidate at 19:53:57.16 +00:33:33.9: ref_mag=13.76 +/- 0.05 new_mean_mag=13.8293 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:29:20.59 -01:24:12.6: 13.63 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.05
Forced photometry filter REJECTED candidate at 19:29:20.59 -01:24:12.6: ref_mag=13.66 +/- 0.05 new_mean_mag=13.5639 delta=0.10 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:35:57.84 -05:34:23.1: 14.55 +/- 0.14 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 20:06:13.32 -04:10:29.5: 13.92 +/- 0.08 detection
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:51:29.72 -02:47:03.1: 15.18 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Forced photometry filter REJECTED candidate at 20:06:13.32 -04:10:29.5: ref_mag=13.85 +/- 0.05 new_mean_mag=13.8361 delta=0.02 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-06-12_04-10-32_20.00sec_5.00C_LIGHT_0226.fits at 19:35:10.05 +01:55:26.4: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:35:57.84 -05:34:23.1: 14.52 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.10
Forced photometry filter REJECTED candidate at 19:35:57.84 -05:34:23.1: ref_mag=14.53 +/- 0.10 new_mean_mag=14.0277 delta=0.51 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:51:29.72 -02:47:03.1: 15.27 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.15
Forced photometry filter KEPT candidate at 19:51:29.72 -02:47:03.1: ref_mag=15.23 +/- 0.15 new_mean_mag=14.2401 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aql-04-Q2b1x1_2026-07-20_02-15-16_20.00sec_4.90C_LIGHT_0290.fits at 19:35:10.05 +01:55:26.4: 15.19 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.21
Forced photometry filter KEPT candidate at 19:35:10.05 +01:55:26.4: ref_mag=15.19 +/- 0.21 new_mean_mag=14.2322 delta=0.96 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out197898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out197760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197819.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: 3s
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Considering the candidate 197677_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197677_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197682_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197682_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197683_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197683_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197688_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197688_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197692_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197692_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197694_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197694_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197709_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197709_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 197711_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197711_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197714_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197714_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197716_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197716_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197725_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197725_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197736_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197736_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197740_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197740_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197744_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197744_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 20:01:32.99 -05:50:02.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 197760_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
Preparing report for the candidate 197760_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
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Considering the candidate 197790_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197790_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 20:01:34.40 -00:11:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197795_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197795_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 19:45:50.79 -02:51:23.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197801_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
Preparing report for the candidate 197801_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
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Considering the candidate 197803_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197803_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197812_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197812_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 197816_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197816_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197817_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197817_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 197819_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
Preparing report for the candidate 197819_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
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Considering the candidate 197834_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197834_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197839_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197839_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197844_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197844_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197849_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197849_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197853_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197853_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 19:39:14.53 -03:11:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197861_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197861_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197865_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197865_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197869_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197869_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197872_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197872_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 20:00:20.79 +02:12:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197879_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197879_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197890_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197890_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
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Considering the candidate 197898_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197898_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 19:51:29.72 -02:47:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 3.987 4233906918487736576 297.87494081953 -02.78424992425 15.2099 14.4925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197905_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197905_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 19:35:10.05 +01:55:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 4.812 4288100884560563328 293.79111484230 +01.92509988998 12.2567 10.4453 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197909_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 197909_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 19:31:50.23 +00:48:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180444_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 180444_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 20:01:47.04 +02:07:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181948_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 181948_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 20:03:20.13 -01:29:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91952_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 91952_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 19:35:29.26 -01:44:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184647_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 184647_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 20:00:08.80 -02:13:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181840_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 181840_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 19:26:09.46 -02:30:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181830_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 181830_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 19:33:28.84 -02:10:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181002_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 181002_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks
**** FOUND 20:07:37.25 -02:27:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180696_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251
The candidate 180696_fd_Aql-04-Q2b1x1_2026-08-04_01-23-14_20.00sec_0.00C_LIGHT_0251 did not pass the final checks