This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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 04 16.4319* 17 02 36.11 +25 51 32.2 11.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0452 Her,2461146.9319,11.34,0.05,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
V0452 Her 20260416.4319 11.34CV 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
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 04 16.4319* 16 41 41.39 +25 43 55.9 14.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2982656,2461146.9319,14.31,0.05,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
DocumentRef: VOTx2982656 20260416.4319 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 16.4319 2461146.9319 14.62 16:48:02.67 +26:12:48.0
46.32193 37.65012 galactic Her Second-epoch detections are separated by 4.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1306430301559420544 | 16:48:02.67 +26:12:48.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.185+/-0.108 (M)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.4319* 16 48 02.67 +26 12 48.0 14.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1306430301559420544,2461146.9319,14.62,0.05,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
Large-amplitude variable Gaia DR2 1306430301559420544 20260416.4319 14.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 04 16.4319* 17 00 33.23 +31 13 22.8 13.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RV Her,2461146.9319,13.46,0.05,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
RV Her 20260416.4319 13.46CV 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
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 04 16.4319* 16 41 59.29 +32 55 27.9 9.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
[D2006] LCD19,2461146.9319,9.64,0.05,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
[D2006] LCD19 20260416.4319 9.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461121.99154078 22.03.2026 11:47:39.123 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
First image: 2461121.99154078 22.03.2026 11:47:39.123 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
Last image: 2461146.93226003 16.04.2026 10:22:17.267 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 21
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 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): 13494
Objects passed selection criteria: 13436
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 9944
Average stars matched: 8204.75 (82.5096 %)
Memory usage VmPeak: 116940 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 06:22:38 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: 2461121.99154078 22.03.2026 11:47:39.123 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
First image: 2461121.99154078 22.03.2026 11:47:39.123 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
Last image: 2461146.93226003 16.04.2026 10:22:17.267 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 57
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 51 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): 66584
Objects passed selection criteria: 66400
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 53015.8
Average stars matched: 47383.2 (89.3758 %)
Memory usage VmPeak: 161100 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 06:24:45 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/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
SExtractor catalog cache: saved Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat to cache
SExtractor catalog cache: saved Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.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/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.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: 2461146.93161727
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits exists and is non-empty
Saving wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits to local_wcs_cache/
'wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits' -> 'local_wcs_cache/wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits'
wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits exists and is non-empty
Saving wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits to local_wcs_cache/
'wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits' -> 'local_wcs_cache/wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits'
wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits exists and is non-empty
Saving wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits to local_wcs_cache/
'wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits' -> 'local_wcs_cache/wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits'
wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits exists and is non-empty
Saving wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits to local_wcs_cache/
'wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits' -> 'local_wcs_cache/wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits (1st reference image)
verification OK: wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 17:00:00.691 +29:59:59.17 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits (1st new image)
verification OK: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
Image size: 936.9'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:59:42.632 +29:59:42.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:00:00.691 +29:59:59.17
Second-epoch image center 16:59:42.632 +29:59:42.26
Angular distance between the image centers 0.0653 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits (2nd new image)
verification OK: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
Image size: 936.9'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:59:40.346 +30:00:20.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:00:00.691 +29:59:59.17
Second-epoch image center 16:59:40.346 +30:00:20.65
Angular distance between the image centers 0.0737 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 16:59:42.632 +29:59:42.26
Second-epoch second image center 16:59:40.346 +30:00:20.65
Angular distance between the image centers 0.01348 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/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits &> /tmp/tmp.ugJchHutcg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits &> /tmp/tmp.EoVD9f9V5Y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits &> /tmp/tmp.gTP0NbNoqA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits &> /tmp/tmp.Z0ARSKK7Ea
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.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_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits and wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.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_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits and wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat
Found non-empty wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits and wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat
The reference image (wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits) and catalog (wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat) found
'wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat' -> 'wcsmag.cat'
Read 11014 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.2437 to 264.3148 deg, Dec +24.2363 to +35.3465 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 245.2437 to 264.3148 deg, Dec 24.2363 to 35.3465 deg
Loaded 9572 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6833 out of 7206 total matches.
Matched with Tycho-2 7206 out of 11014 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.952524
a=0.000000 b=1.000000 c=22.952524
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
2.1 pix Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
3.4 pix fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
3.4 pix fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
Limiting magnitude estimates:
15.3 mag. Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
15.3 mag. Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
15.1 mag. fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
15.2 mag. fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (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.ugJchHutcg (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/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits' -> 'wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
WCS_IMAGE_NAME=wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
WCS-calibrated image found: wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
Checking if the catalog wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat corresponding to the image wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits alredy exist and is non-empty...
Catalog wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat corresponding to the image wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
WCS catalog name: wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=839, passed=11014
Got 11014 stars (including 10161 good ones) from the SExtractor catalog wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat
util/solve_plate_with_UCAC5 got 11014 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10829 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits -region wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.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.EoVD9f9V5Y (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/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits' -> 'wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
WCS_IMAGE_NAME=wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
WCS-calibrated image found: wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
Checking if the catalog wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat corresponding to the image wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits alredy exist and is non-empty...
Catalog wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat corresponding to the image wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
WCS catalog name: wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=848, passed=10793
Got 10793 stars (including 9927 good ones) from the SExtractor catalog wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat
util/solve_plate_with_UCAC5 got 10793 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10620 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10620 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits -region wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.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.gTP0NbNoqA (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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
WCS_IMAGE_NAME=wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
WCS-calibrated image found: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
Checking if the catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
WCS catalog name: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1128, passed=14416
Got 14416 stars (including 13278 good ones) from the SExtractor catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat
util/solve_plate_with_UCAC5 got 14416 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 14137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 14137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 14134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 971 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits -region wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.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.Z0ARSKK7Ea (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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
WCS-calibrated image found: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
Checking if the catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
WCS catalog name: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1091, passed=14357
Got 14357 stars (including 13255 good ones) from the SExtractor catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat
util/solve_plate_with_UCAC5 got 14357 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 14097 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 14096 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 14096 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits -region wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.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_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits'
Saving fully-calibrated image wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits'
Saving fully-calibrated image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits'
Saving fully-calibrated image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits'
Preparing the HTML report for the field Her-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out01268.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22453_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22453_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:13:57.34 +28:48:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22485_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22485_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:13:19.98 +28:45:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.986 4575441858865715968 258.33325133456 +28.75688503501 12.1709 11.7182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22605_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22605_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:12:30.28 +30:27:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.082 1309133592627932416 258.12600939191 +30.45246275013 10.6041 9.1711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22637_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22637_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:57:54.87 +29:26:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.449 1309531718916739072 254.47849206055 +29.43526879140 11.9947 11.4172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22700_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22700_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:50:32.29 +29:46:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22702_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22702_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:05:52.31 +27:02:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.608 4574838639298381312 256.46745848901 +27.03852084586 12.3288 11.6194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22745_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22745_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:54:44.26 +28:48:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.341 1307984839198341760 253.68451548959 +28.80873963064 12.0488 11.3430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22769_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22769_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:57:00.30 +29:17:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.171 1309505635579117824 254.25126873251 +29.29592769483 12.0127 11.3553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22778_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22778_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:57:46.14 +29:52:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.538 1309559996981501312 254.44209618748 +29.87432153592 12.0125 11.2666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22784_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22784_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:59:16.78 +28:41:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.029 1308669220763972096 254.81992171047 +28.68903451376 12.1330 11.6595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22793_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22793_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:43:05.30 +26:12:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.864 1301242702616262912 250.77254793749 +26.20450153605 12.1145 11.3965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22806_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22806_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:02:55.46 +29:03:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.488 1308743437799086848 255.73092822431 +29.06628178737 11.9823 11.2151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22834_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22834_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:10:53.83 +29:31:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.780 1308926987521394816 257.72411440498 +29.52576342382 12.3017 11.7666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22855_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22855_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:54:02.72 +28:29:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.557 1307947631898350720 253.51117752473 +28.48823852203 12.2040 11.7050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22887_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 22887_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:43:41.13 +26:10:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.294 1301230199968745088 250.92203694043 +26.18086948335 12.3028 11.6699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 01268_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
Preparing report for the candidate 01268_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 19s
Prepared the HTML report for the field Her-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
17:02:36.11 +25:51:32.2
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/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
SExtractor catalog cache: saved Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat to cache
SExtractor catalog cache: saved Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
Creating symlink local_wcs_cache/wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
Creating symlink local_wcs_cache/wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
Creating symlink local_wcs_cache/wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.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_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits exists and is non-empty
wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits exists and is non-empty
wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits exists and is non-empty
wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits (1st reference image)
verification OK: wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 17:00:00.691 +29:59:59.17 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits (1st new image)
verification OK: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
Image size: 936.9'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:59:42.632 +29:59:42.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:00:00.691 +29:59:59.17
Second-epoch image center 16:59:42.632 +29:59:42.26
Angular distance between the image centers 0.0653 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits (2nd new image)
verification OK: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
Image size: 936.9'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:59:40.346 +30:00:20.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:00:00.691 +29:59:59.17
Second-epoch image center 16:59:40.346 +30:00:20.65
Angular distance between the image centers 0.0737 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 16:59:42.632 +29:59:42.26
Second-epoch second image center 16:59:40.346 +30:00:20.65
Angular distance between the image centers 0.01348 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/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits &> /tmp/tmp.yS2sO9W09M
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits &> /tmp/tmp.qdajir4jb3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits &> /tmp/tmp.9gipMupE4i
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits &> /tmp/tmp.mjiN9iThcp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.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_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits and wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.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_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits and wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat
Found non-empty wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits and wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat
The reference image (wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits) and catalog (wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat) found
'wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat' -> 'wcsmag.cat'
Read 72123 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 245.2351 to 264.3431 deg, Dec +24.2117 to +35.3511 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 245.2351 to 264.3431 deg, Dec 24.2117 to 35.3511 deg
Loaded 9612 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6440 out of 7388 total matches.
Matched with Tycho-2 7388 out of 72123 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.815895
a=0.000000 b=1.000000 c=22.815895
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
1.9 pix Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
3.3 pix fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
3.3 pix fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
Limiting magnitude estimates:
15.5 mag. Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
15.5 mag. Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
15.4 mag. fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
15.4 mag. fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (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.yS2sO9W09M (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/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits' -> 'wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
WCS_IMAGE_NAME=wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
WCS-calibrated image found: wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
Checking if the catalog wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat corresponding to the image wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits alredy exist and is non-empty...
Catalog wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat corresponding to the image wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
WCS catalog name: wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=3961, passed=72111
Got 72111 stars (including 68033 good ones) from the SExtractor catalog wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat
util/solve_plate_with_UCAC5 got 72111 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 70856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 70855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 70854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits -region wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.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.qdajir4jb3 (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/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits' -> 'wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
WCS_IMAGE_NAME=wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
WCS-calibrated image found: wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
Checking if the catalog wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat corresponding to the image wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits alredy exist and is non-empty...
Catalog wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat corresponding to the image wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
WCS catalog name: wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=3901, passed=70840
Got 70840 stars (including 66824 good ones) from the SExtractor catalog wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat
util/solve_plate_with_UCAC5 got 70840 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 69806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 69804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 69805 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits -region wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.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.9gipMupE4i (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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
WCS_IMAGE_NAME=wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
WCS-calibrated image found: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
Checking if the catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
WCS catalog name: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=6357, passed=60673
Got 60673 stars (including 54279 good ones) from the SExtractor catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat
util/solve_plate_with_UCAC5 got 60673 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 59449 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 59449 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 59449 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits -region wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.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.mjiN9iThcp (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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
WCS-calibrated image found: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
Checking if the catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat corresponding to the image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
WCS catalog name: wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=6062, passed=59923
Got 59923 stars (including 53827 good ones) from the SExtractor catalog wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat
util/solve_plate_with_UCAC5 got 59923 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 58899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 58899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 58893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 972 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits -region wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.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_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/wcs_Her-04-Q2b1x1_2026-03-22_06-47-39_20.00sec_-15.00C_LIGHT_0397.fits
Saving fully-calibrated image wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/wcs_Her-04-Q2b1x1_2026-03-22_06-48-32_20.00sec_-15.00C_LIGHT_0398.fits
Saving fully-calibrated image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/wcs_fd_Her-04-Q2b1x1_2026-04-16_05-21-21_20.00sec_-4.90C_LIGHT_0414.fits
Saving fully-calibrated image wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.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_2026-04-16_CI_Her-04-Q2b1x1_052304_TTUQ2b1x1_1256_HZv2sGY0/wcs_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415.fits
Preparing the HTML report for the field Her-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out100115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out50724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99544.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 402s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 86108_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 86108_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:08:13.22 +29:29:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86112_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
Preparing report for the candidate 86112_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
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Considering the candidate 86113_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 86113_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:18:44.71 +30:34:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95403_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 95403_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:16:53.52 +26:08:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97710_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 97710_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:17:58.83 +26:57:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99097_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 99097_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 99490_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 99490_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:13:03.29 +26:13:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 3.662 4573802315230553600 258.26416594471 +26.22448635960 15.1891 14.7751 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99540_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 99540_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:19:36.15 +25:47:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.114 4573585230403563136 259.90057904863 +25.79263780680 14.3837 13.2585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99544_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
Preparing report for the candidate 99544_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
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Considering the candidate 99827_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 99827_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:13:22.10 +33:44:49.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)
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Considering the candidate 99858_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 99858_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:12:51.85 +27:13:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.316 4574726798350471296 258.21585077490 +27.23279593348 14.9857 14.4882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99863_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 99863_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:12:29.20 +26:00:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 2.271 4573746205777605888 258.12129944553 +26.00251807543 15.1259 14.6139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99967_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 99967_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:11:07.55 +31:37:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100115_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 100115_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:20:13.43 +32:25:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.696 1333755025228416384 260.05607856589 +32.43148788291 15.0319 14.5468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100167_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 100167_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:18:12.77 +25:59:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.250 4573605433929859712 259.55352147842 +25.99818578680 14.9068 14.4188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100169_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 100169_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:06:46.79 +29:30:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100243_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 100243_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:19:24.31 +27:53:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 0.513 4574468516197936128 259.85137289345 +27.88548788285 14.7776 14.3381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100387_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 100387_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:19:52.88 +26:54:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100451_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 100451_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:58:33.83 +26:38:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 3.141 1306665807499451904 254.64007353158 +26.63595152500 14.6700 13.8586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100521_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 100521_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:18:01.06 +26:39:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100836_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 100836_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:13:11.58 +28:27:23.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)
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Considering the candidate 100958_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 100958_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:10:24.93 +30:52:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 1.667 1309348478431747456 257.60333883032 +30.87846944692 14.4661 13.4433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101119_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 101119_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:06:51.65 +33:16:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 0.685 1334607078020167296 256.71505167806 +33.26680480099 15.5604 14.8717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101127_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 101127_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:14:37.20 +30:09:21.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)
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Considering the candidate 101261_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 101261_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:00:23.85 +30:45:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 2.440 1309895038789759744 255.09862533921 +30.76412770847 14.5404 13.4286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101462_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 101462_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 16:56:42.25 +25:57:31.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)
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Considering the candidate 101582_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 101582_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks
**** FOUND 17:06:32.67 +32:27:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.397 1334499325880412032 256.63621759100 +32.46288001928 14.8959 14.2743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50724_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
Preparing report for the candidate 50724_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
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Considering the candidate 60469_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
Preparing report for the candidate 60469_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
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Considering the candidate 07396_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415
The candidate 07396_fd_Her-04-Q2b1x1_2026-04-16_05-22-17_20.00sec_-4.90C_LIGHT_0415 did not pass the final checks