This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV
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 03 30.2074 2461129.7074 11.95 16:41:34.73 +36:25:15.7
58.95310 40.93033 galactic Her Second-epoch detections are separated by 5.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1328057355974348672 | 16:41:32.53 +36:24:42.5 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G5/8Ib 1947ApJ...105..204P NGC 6205 199
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.2075* 16 41 34.73 +36 25 15.7 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1328057355974348672,2461129.7074,11.95,0.05,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
Gaia DR3 1328057355974348672 20260330.2074 11.95CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:41:34.73 +36:25:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20_00sec_-10_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20_00sec_-10_00C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20_00sec_-10_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20_00sec_-10_00C_LIGHT_0186_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.2074 2461129.7074 12.07 16:41:53.38 +36:26:26.8
58.98820 40.87037 galactic Her Second-epoch detections are separated by 4.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J250.4754+36.4358 | 16:41:54.06 +36:26:27.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5III/V 1947ApJ...105..204P NGC 6205 993 J-Ks=0.478+/- (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.2075* 16 41 53.38 +36 26 26.8 12.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J250.4754+36.4358,2461129.7074,12.07,0.05,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
ATO J250.4754+36.4358 20260330.2074 12.07CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:41:53.38 +36:26:26.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20_00sec_-10_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20_00sec_-10_00C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20_00sec_-10_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20_00sec_-10_00C_LIGHT_0186_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.2074 2461129.7074 12.16 16:41:48.92 +36:25:33.8
58.96666 40.88360 galactic Her Second-epoch detections are separated by 7.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | V1578 Her | 16:41:47.01 +36:25:57.5 (Gaia DR3) | SR (local) | : (local) | Gaia3var=NOT_AVAILABLE SpType: G2/5Ib 1947ApJ...105..204P NGC 6205 835
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.2075* 16 41 48.92 +36 25 33.8 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1578 Her,2461129.7074,12.16,0.05,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
V1578 Her 20260330.2074 12.16CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:41:48.92 +36:25:33.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20_00sec_-10_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20_00sec_-10_00C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20_00sec_-10_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png resample_wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20_00sec_-10_00C_LIGHT_0186_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461121.97230774 22.03.2026 11:19:57.389 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
First image: 2461121.97230774 22.03.2026 11:19:57.389 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
Last image: 2461129.70777068 30.03.2026 04:59:01.387 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.40
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8747
Objects passed selection criteria: 8694
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 5547
Average stars matched: 5332.5 (96.133 %)
Memory usage VmPeak: 114876 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Mar 30 00:03:35 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: 2461121.97230774 22.03.2026 11:19:57.389 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
First image: 2461121.97230774 22.03.2026 11:19:57.389 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
Last image: 2461129.70777068 30.03.2026 04:59:01.387 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.13
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: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 52509
Objects passed selection criteria: 52367
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 35083.8
Average stars matched: 33413 (95.2378 %)
Memory usage VmPeak: 154464 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Mar 30 00:04:21 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
SExtractor catalog cache: saved CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat to cache
SExtractor catalog cache: saved CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.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/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.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: 2461129.70712461
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits exists and is non-empty
Saving wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits to local_wcs_cache/
'wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits' -> 'local_wcs_cache/wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits'
wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits exists and is non-empty
Saving wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits to local_wcs_cache/
'wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits' -> 'local_wcs_cache/wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits'
wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits exists and is non-empty
Saving wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits to local_wcs_cache/
'wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits' -> 'local_wcs_cache/wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits'
wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits exists and is non-empty
Saving wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits to local_wcs_cache/
'wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits' -> 'local_wcs_cache/wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:21:48.591 +38:00:08.03
Second-epoch image center 16:21:43.593 +38:02:36.66
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:21:48.591 +38:00:08.03
Second-epoch image center 16:21:43.286 +38:01:53.90
Angular distance between the image centers 0.03 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 16:21:43.593 +38:02:36.66
Second-epoch second image center 16:21:43.286 +38:01:53.90
Angular distance between the image centers 0.01192 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits &> /tmp/tmp.k8FWYL41zE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits &> /tmp/tmp.px0sdPvSZ3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits &> /tmp/tmp.2QI9wciRVp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits &> /tmp/tmp.lXvg89mBfz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
Calibrating the magnitude scale
Found non-empty wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.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_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits and wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat
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_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits and wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat
Found non-empty wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits and wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat
The reference image (wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits) and catalog (wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat) found
'wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5259 out of 10322 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.951996
a=0.000000 b=1.000000 c=22.951996
From vast_summary.log: estimated ref. image limiting mag.: -7.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.55
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.55
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
2.0 pix CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
2.4 pix fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
2.4 pix fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
Limiting magnitude estimates:
15.5 mag. CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
15.5 mag. CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
13.3 mag. fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
13.3 mag. fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 10.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.k8FWYL41zE (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits' -> 'wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
WCS_IMAGE_NAME=wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
WCS-calibrated image found: wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
Checking if the catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat corresponding to the image wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits alredy exist and is non-empty...
Catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat corresponding to the image wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
WCS catalog name: wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=710, passed=10322
Got 10322 stars (including 9592 good ones) from the SExtractor catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat
util/solve_plate_with_UCAC5 got 10322 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits -region wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.px0sdPvSZ3 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits' -> 'wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
WCS_IMAGE_NAME=wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
WCS-calibrated image found: wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
Checking if the catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat corresponding to the image wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits alredy exist and is non-empty...
Catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat corresponding to the image wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
WCS catalog name: wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=714, passed=10255
Got 10255 stars (including 9525 good ones) from the SExtractor catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat
util/solve_plate_with_UCAC5 got 10255 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits -region wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2QI9wciRVp (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_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.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_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
WCS_IMAGE_NAME=wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
WCS-calibrated image found: wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
Checking if the catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits alredy exist and is non-empty...
Catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
WCS catalog name: wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=181, passed=2554
Got 2554 stars (including 2371 good ones) from the SExtractor catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat
util/solve_plate_with_UCAC5 got 2554 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
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
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits -region wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.lXvg89mBfz (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_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.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_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
Checking if the catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
WCS catalog name: wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=182, passed=2560
Got 2560 stars (including 2374 good ones) from the SExtractor catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat
util/solve_plate_with_UCAC5 got 2560 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (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 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
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
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits -region wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits'
Saving fully-calibrated image wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits'
Saving fully-calibrated image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits'
Saving fully-calibrated image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits'
Preparing the HTML report for the field CrB-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field CrB-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
SExtractor catalog cache: saved CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat to cache
SExtractor catalog cache: saved CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
Creating symlink local_wcs_cache/wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
Creating symlink local_wcs_cache/wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
Creating symlink local_wcs_cache/wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.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_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits exists and is non-empty
wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits exists and is non-empty
wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits exists and is non-empty
wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:21:48.591 +38:00:08.03
Second-epoch image center 16:21:43.593 +38:02:36.66
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:21:48.591 +38:00:08.03
Second-epoch image center 16:21:43.286 +38:01:53.90
Angular distance between the image centers 0.03 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 16:21:43.593 +38:02:36.66
Second-epoch second image center 16:21:43.286 +38:01:53.90
Angular distance between the image centers 0.01192 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits &> /tmp/tmp.bjCIXin6Kn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits &> /tmp/tmp.Oki1dbbH2C
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits &> /tmp/tmp.8FzaF42iVg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits &> /tmp/tmp.gVhrBkH1p7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
Calibrating the magnitude scale
Found non-empty wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.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_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits and wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat
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_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits and wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat
Found non-empty wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits and wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat
The reference image (wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits) and catalog (wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat) found
'wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5285 out of 61628 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.839470
a=0.000000 b=1.000000 c=22.839470
From vast_summary.log: estimated ref. image limiting mag.: -7.13
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.71
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.71
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 18 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
1.9 pix CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
2.2 pix fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
2.2 pix fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
Limiting magnitude estimates:
15.7 mag. CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
15.7 mag. CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
13.7 mag. fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
13.7 mag. fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.bjCIXin6Kn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits' -> 'wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
WCS_IMAGE_NAME=wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
WCS-calibrated image found: wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
Checking if the catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat corresponding to the image wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits alredy exist and is non-empty...
Catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat corresponding to the image wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
WCS catalog name: wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=3241, passed=61610
Got 61610 stars (including 58251 good ones) from the SExtractor catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat
util/solve_plate_with_UCAC5 got 61610 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits -region wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Oki1dbbH2C (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits' -> 'wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
WCS_IMAGE_NAME=wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
WCS-calibrated image found: wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
Checking if the catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat corresponding to the image wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits alredy exist and is non-empty...
Catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat corresponding to the image wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
WCS catalog name: wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat
SExtractor catalog parsing summary: zero_flux=11, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=3229, passed=61566
Got 61566 stars (including 58229 good ones) from the SExtractor catalog wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat
util/solve_plate_with_UCAC5 got 61566 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits -region wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8FzaF42iVg (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_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.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_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
WCS_IMAGE_NAME=wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
WCS-calibrated image found: wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
Checking if the catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits alredy exist and is non-empty...
Catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
WCS catalog name: wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=462, passed=16546
Got 16546 stars (including 16056 good ones) from the SExtractor catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat
util/solve_plate_with_UCAC5 got 16546 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
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
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits -region wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.gVhrBkH1p7 (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_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.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_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
Checking if the catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
WCS catalog name: wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=458, passed=16845
Got 16845 stars (including 16368 good ones) from the SExtractor catalog wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat
util/solve_plate_with_UCAC5 got 16845 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (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 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
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
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits -region wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/wcs_CrB-01-Q2b1x1_2026-03-22_06-19-57_20.00sec_-15.00C_LIGHT_0372.fits
Saving fully-calibrated image wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/wcs_CrB-01-Q2b1x1_2026-03-22_06-20-39_20.00sec_-15.00C_LIGHT_0373.fits
Saving fully-calibrated image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.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_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-58-05_20.00sec_-10.00C_LIGHT_0186.fits
Saving fully-calibrated image wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.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_2026-03-30_CI_CrB-01-Q2b1x1_000120_TTUQ2b1x1_28897_UazGFQNV/wcs_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187.fits
Preparing the HTML report for the field CrB-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out44163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out76841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out76891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out76853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77150.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 76080_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 76080_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:19:02.75 +40:10:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76841_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 76841_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:41:50.18 +36:24:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.689 1328056703145773696 250.45956308908 +36.40430515924 11.5412 10.6739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 76853_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
Preparing report for the candidate 76853_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
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Considering the candidate 76891_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 76891_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:41:32.39 +36:24:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 2.803 1328057351677265920 250.38552724416 +36.41181478855 11.7330 10.9049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 76896_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
Preparing report for the candidate 76896_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
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Considering the candidate 76975_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 76975_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:11:39.30 +36:24:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77019_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 77019_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:11:36.97 +36:25:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77045_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 77045_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:44:06.04 +41:39:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77048_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 77048_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:41:44.87 +36:30:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.982 1328059726803469312 250.43686742355 +36.51425985115 12.0734 11.2700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77059_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 77059_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 15:51:21.75 +35:40:19.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 77081_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 77081_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:41:30.58 +36:29:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77150_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
Preparing report for the candidate 77150_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
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Considering the candidate 77192_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 77192_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 77485_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 77485_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 15:59:05.24 +36:55:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77547_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 77547_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:25:01.75 +39:09:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77688_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 77688_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:41:30.70 +36:30:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43746_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 43746_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks
**** FOUND 16:41:27.22 +36:28:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44163_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187
The candidate 44163_fd_CrB-01-Q2b1x1_2026-03-29_23-59-01_20.00sec_-10.00C_LIGHT_0187 did not pass the final checks