This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 23.3779 2461153.8779 10.91 19:29:20.47 -18:53:33.6
19.83288 -16.63491 galactic Sgr Second-epoch detections are separated by 0.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.8 Flora 3 -2 4 11.1 -0 -0
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits at 19:29:20.47 -18:53:33.6: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits at 19:29:20.47 -18:53:33.6: 15.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.8779,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.3779 10.91CV 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 23.3779 2461153.8779 12.35 19:27:11.01 -16:05:25.3
22.27506 -15.02321 galactic Sgr Second-epoch detections are separated by 2.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.409 Aspasia -1 1 1 12.2 -0 -0
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits at 19:27:11.01 -16:05:25.3: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits at 19:27:11.01 -16:05:25.3: 15.31 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.8779,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.3779 12.35CV 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 23.3779 2461153.8779 13.59 19:45:53.00 -17:07:37.7
23.18516 -19.53855 galactic Sgr Second-epoch detections are separated by 2.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.60 Echo 2 0 2 13.9 -0 -0
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits at 19:45:53.00 -17:07:37.7: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits at 19:45:53.00 -17:07:37.7: 15.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.8779,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.3779 13.59CV 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: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461153.87915472 23.04.2026 09:05:48.968 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.53
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: 4 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): 10467
Objects passed selection criteria: 10465
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 9982.75
Average stars matched: 9317.75 (93.3385 %)
Memory usage VmPeak: 115884 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 04:08:38 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: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461153.87915472 23.04.2026 09:05:48.968 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 94
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.17
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: 55 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): 105008
Objects passed selection criteria: 104833
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 98623.2
Average stars matched: 88505.8 (89.7413 %)
Memory usage VmPeak: 2129068 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 04:11:41 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/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.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: 2461153.87669644
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_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits (1st reference image)
verification OK: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Image size: 938.1'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:22.678 -18:00:40.27 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits (1st new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
Image size: 938.5'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:29.151 -18:01:52.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:29.151 -18:01:52.77
Angular distance between the image centers 0.0326 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits (2nd new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
Image size: 938.2'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:27.259 -18:02:03.52 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:27.259 -18:02:03.52
Angular distance between the image centers 0.0294 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:33:29.151 -18:01:52.77
Second-epoch second image center 19:33:27.259 -18:02:03.52
Angular distance between the image centers 0.00807 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/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.erd1ZNAmFH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.lRBxuVdwAR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits &> /tmp/tmp.9ncpaXJHUF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits &> /tmp/tmp.5FVXxPW7hJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 11017 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7685 to 301.7245 deg, Dec -23.3021 to -12.5136 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 284.7685 to 301.7245 deg, Dec -23.3021 to -12.5136 deg
Loaded 13778 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): 8233 out of 8546 total matches.
Matched with Tycho-2 8546 out of 11017 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.784657
a=0.000000 b=1.000000 c=22.784657
From vast_summary.log: estimated ref. image limiting mag.: -8.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.25
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11017 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7685 to 301.7245 deg, Dec -23.3021 to -12.5136 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 284.7685 to 301.7245 deg, Dec -23.3021 to -12.5136 deg
Loaded 13778 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): 8233 out of 8546 total matches.
Matched with Tycho-2 8546 out of 11017 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -> calib.txt_param_ref_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits (aperture=6.5)
Read 13469 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7687 to 301.7265 deg, Dec -23.3084 to -12.5632 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 284.7687 to 301.7265 deg, Dec -23.3084 to -12.5632 deg
Loaded 13734 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): 9218 out of 9683 total matches.
Matched with Tycho-2 9683 out of 13469 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -> calib.txt_param_ref_wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.6 pix fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
2.4 pix fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
2.5 pix wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Limiting magnitude estimates:
14.3 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.6 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
14.1 mag. fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
14.3 mag. fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.4 (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.erd1ZNAmFH (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=800, passed=11017
Got 11017 stars (including 10207 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 11017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 10657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 959 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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.lRBxuVdwAR (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/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1081, passed=13469
Got 13469 stars (including 12369 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 13469 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13041 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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 13040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 13040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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.9ncpaXJHUF (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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=636, passed=9964
Got 9964 stars (including 9319 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat
util/solve_plate_with_UCAC5 got 9964 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 9742 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 9742 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 9741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.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.5FVXxPW7hJ (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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=739, passed=11589
Got 11589 stars (including 10841 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat
util/solve_plate_with_UCAC5 got 11589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 11313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 11313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 11313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.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_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits'
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out22304.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 22294_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 22294_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:16:31.56 -18:01:35.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22304_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
Preparing report for the candidate 22304_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22331_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 22331_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:29:19.19 -15:11:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22335_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 22335_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:06:13.13 -15:49:53.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22346_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 22346_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:21:33.26 -15:55:33.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01564_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 01564_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:13:27.08 -21:33:39.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Sgr-03-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 ####
19:29:20.47 -18:53:33.6
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/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.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_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits (1st reference image)
verification OK: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Image size: 938.1'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:22.678 -18:00:40.27 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits (1st new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
Image size: 938.5'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:29.151 -18:01:52.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:29.151 -18:01:52.77
Angular distance between the image centers 0.0326 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits (2nd new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
Image size: 938.2'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:27.259 -18:02:03.52 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:27.259 -18:02:03.52
Angular distance between the image centers 0.0294 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:33:29.151 -18:01:52.77
Second-epoch second image center 19:33:27.259 -18:02:03.52
Angular distance between the image centers 0.00807 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/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.GgrK6ekkXh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.sOqIFaz9ZE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits &> /tmp/tmp.lAqR8IsnHm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits &> /tmp/tmp.6yxFaRpZbk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 101850 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 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 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 deg
Loaded 13790 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): 10156 out of 11996 total matches.
Matched with Tycho-2 11996 out of 101850 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547522
a=0.000000 b=1.000000 c=22.547522
From vast_summary.log: estimated ref. image limiting mag.: -8.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 101850 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 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 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 deg
Loaded 13790 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): 10156 out of 11996 total matches.
Matched with Tycho-2 11996 out of 101850 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -> calib.txt_param_ref_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits (aperture=4.8)
Read 138134 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7420 to 301.7832 deg, Dec -23.3118 to -12.5402 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 284.7420 to 301.7832 deg, Dec -23.3118 to -12.5402 deg
Loaded 13812 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): 9867 out of 12175 total matches.
Matched with Tycho-2 12175 out of 138134 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -> calib.txt_param_ref_wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.4 pix fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
2.3 pix fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
2.4 pix wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Limiting magnitude estimates:
14.4 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.7 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
14.2 mag. fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
14.4 mag. fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.6 (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.GgrK6ekkXh (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=8404, passed=101839
Got 101839 stars (including 93311 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 101839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 98878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 98875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 98875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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.sOqIFaz9ZE (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/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=12676, passed=138124
Got 138124 stars (including 125221 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 138124 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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.lAqR8IsnHm (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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=7362, passed=92155
Got 92155 stars (including 84684 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat
util/solve_plate_with_UCAC5 got 92155 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 90538 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 90538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 90538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.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.6yxFaRpZbk (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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=8685, passed=107032
Got 107032 stars (including 98211 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat
util/solve_plate_with_UCAC5 got 107032 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 104374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 104372 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 104371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.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_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-02-16_20.00sec_-4.90C_LIGHT_0238.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.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_2026-04-23_CI_Sgr-03-Q2b1x1_040626_TTUQ2b1x1_2031852_xsFRhhIL/wcs_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239.fits
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out148181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out148553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149020.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 148181_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148181_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:28:32.93 -20:11:25.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 148195_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148195_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:21:43.66 -18:48:15.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 148201_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148201_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:18:11.53 -16:03:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.100 4183969020198418944 289.54805343838 -16.06422471222 13.3188 12.5824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148202_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148202_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:11:35.08 -16:53:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.662 4087923969406304512 287.89557346034 -16.88674833430 12.5379 11.3382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148204_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148204_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:08:47.23 -14:12:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 3.588 4185356779987490816 287.19612905305 -14.21509550244 13.6419 12.7605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148205_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148205_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:34:17.53 -13:54:24.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)
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Considering the candidate 148213_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148213_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:07:16.16 -15:24:41.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)
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Considering the candidate 148226_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148226_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:15:37.98 -14:00:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148233_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148233_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:51:44.99 -18:06:21.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)
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Considering the candidate 148240_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148240_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 148242_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148242_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:33:47.28 -14:25:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148246_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148246_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:36:30.66 -13:50:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148251_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148251_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:16:26.53 -14:53:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.212 4185120591140122752 289.11044947482 -14.89386428996 13.1603 12.3641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148253_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148253_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:37:02.06 -16:18:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.521 4180387296650575488 294.25829752032 -16.30529348906 13.7672 13.1181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148274_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148274_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:05:22.34 -20:23:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148281_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148281_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:06:29.87 -14:47:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.812 4089256160866339840 286.62370153494 -14.78599580028 13.0892 12.5102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148307_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148307_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:10:24.46 -15:40:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148312_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148312_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:19:25.11 -18:47:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148314_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148314_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:11:03.11 -13:47:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148327_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148327_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:13:04.90 -15:18:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.662 4184998064313463936 288.27087569508 -15.31069967582 13.2210 12.4292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148331_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148331_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:17:19.06 -19:53:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.405 4083039041087014912 289.32954642660 -19.89471227030 12.8550 12.1004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148388_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148388_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:29:20.26 -18:53:31.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 148546_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148546_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:29:32.79 -21:19:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148553_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
Preparing report for the candidate 148553_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
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Considering the candidate 148680_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148680_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:38:19.95 -14:55:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148783_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148783_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:46:26.58 -19:44:31.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 148819_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148819_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:30:03.13 -19:22:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148893_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148893_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:41:04.27 -15:24:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.848 4182034914823467008 295.26779405389 -15.40798550934 13.5106 12.8358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148914_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148914_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:06:46.44 -17:27:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148947_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148947_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:17:41.26 -17:21:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148974_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148974_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:08:11.41 -16:38:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148993_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 148993_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:05:40.42 -18:17:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149020_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
Preparing report for the candidate 149020_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
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Considering the candidate 149033_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149033_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:45:43.24 -13:46:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149046_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149046_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:07:15.57 -19:44:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.382 4082499563148945664 286.81498468710 -19.73532401957 13.7900 13.1848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149072_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149072_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:14:01.02 -18:52:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.866 4084116498073314432 288.50399726845 -18.87633474444 13.2752 12.3030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149074_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149074_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:21:37.04 -17:19:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149083_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149083_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:47:26.39 -14:34:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149085_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149085_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:10:20.15 -17:45:21.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 149095_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149095_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:06:17.53 -20:30:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149102_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149102_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:38:02.00 -15:44:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.861 4181955578188402048 294.50797570919 -15.73966352938 13.8582 13.1870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149115_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149115_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:08:48.38 -21:46:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.151 4081210385758893312 287.20094825447 -21.76748748586 13.9379 13.3305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149117_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149117_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:49:57.52 -14:54:08.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)
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Considering the candidate 149127_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149127_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:20:04.19 -14:12:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149132_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149132_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:36:51.65 -14:19:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 0.323 4182960703615808128 294.21511566536 -14.33238863357 14.4986 13.9058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149166_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 149166_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:32:24.13 -19:42:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114202_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 114202_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:08:22.59 -17:11:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48852_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 48852_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:16:31.56 -18:01:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12226_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 12226_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:13:27.06 -21:33:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124612_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 124612_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:37:52.14 -14:08:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112656_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 112656_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:26:18.46 -19:10:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54430_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 54430_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:49:31.40 -17:40:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07863_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 07863_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:28:04.96 -22:14:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117252_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 117252_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks
**** FOUND 19:27:04.43 -14:50:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116965_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239
The candidate 116965_fd_Sgr-03-Q2b1x1_2026-04-23_04-05-48_20.00sec_-5.00C_LIGHT_0239 did not pass the final checks