This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG
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 05 03.3480 2461163.8480 10.59 19:36:43.31 -18:43:51.7
20.71691 -18.17282 galactic Sgr Second-epoch detections are separated by 0.2" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.8 Flora 1 -0 1 10.9 -0 -0
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:36:43.31 -18:43:51.7: 13.72 +/- 0.09 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:36:43.31 -18:43:51.7: 13.50 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.05
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,2461163.8480,10.59,0.05,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 20260503.3480 10.59CV 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
Mean magnitude and position on the discovery images:
2026 05 03.3480 2461163.8480 11.95 19:33:34.74 -14:51:48.6
24.09609 -15.91726 galactic Sgr Second-epoch detections are separated by 0.2" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.409 Aspasia -0 1 1 12.0 -0 -0
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:33:34.74 -14:51:48.6: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:33:34.74 -14:51:48.6: 15.46 +/- 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,2461163.8480,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260503.3480 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.3480 2461163.8480 13.82 19:50:49.31 -16:39:49.0
24.13655 -20.43913 galactic Sgr Second-epoch detections are separated by 2.8" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.60 Echo 3 -0 3 13.8 -0 -0
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:50:49.31 -16:39:49.0: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:50:49.31 -16:39:49.0: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461163.8480,13.82,0.05,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 20260503.3480 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461121.98536419 22.03.2026 11:38:45.466 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
First image: 2461121.98536419 22.03.2026 11:38:45.466 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
Last image: 2461163.84829299 03.05.2026 08:21:22.514 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.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.: -8.27
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): 11706
Objects passed selection criteria: 11672
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 9096.5
Average stars matched: 8295.25 (91.1917 %)
Memory usage VmPeak: 118224 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 03:23:58 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461121.98536419 22.03.2026 11:38:45.466 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
First image: 2461121.98536419 22.03.2026 11:38:45.466 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
Last image: 2461163.84829299 03.05.2026 08:21:22.514 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 85
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
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: 25 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): 111900
Objects passed selection criteria: 111732
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 89584.8
Average stars matched: 84778.5 (94.635 %)
Memory usage VmPeak: 1949392 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 03:26:55 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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.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: 2461163.84778581
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits'
wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits (1st reference image)
verification OK: wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
Image size: 942.0'x627.4' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:19.463 -17:59:59.67 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits (1st new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
Image size: 938.6'x624.7' 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: 19:33:41.779 -17:56:57.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:19.463 -17:59:59.67
Second-epoch image center 19:33:41.779 -17:56:57.34
Angular distance between the image centers 0.1019 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits (2nd new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
Image size: 938.6'x624.7' 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: 19:33:42.386 -17:57:02.58 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:19.463 -17:59:59.67
Second-epoch image center 19:33:42.386 -17:57:02.58
Angular distance between the image centers 0.1033 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 19:33:41.779 -17:56:57.34
Second-epoch second image center 19:33:42.386 -17:57:02.58
Angular distance between the image centers 0.00281 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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits &> /tmp/tmp.2B5dxYuKEd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits &> /tmp/tmp.3uPdbOE4ZR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits &> /tmp/tmp.Zvvt90DSDJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits &> /tmp/tmp.8BhtIQL4iU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits and wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits and wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits and wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat' -> 'wcsmag.cat'
Read 13915 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7687 to 301.7264 deg, Dec -23.2929 to -12.5406 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 301.7264 deg, Dec -23.2929 to -12.5406 deg
Loaded 13742 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): 9348 out of 9835 total matches.
Matched with Tycho-2 9835 out of 13915 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.814700
a=0.000000 b=1.000000 c=22.814700
From vast_summary.log: estimated ref. image limiting mag.: -8.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.54
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 13915 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7687 to 301.7264 deg, Dec -23.2929 to -12.5406 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 301.7264 deg, Dec -23.2929 to -12.5406 deg
Loaded 13742 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): 9348 out of 9835 total matches.
Matched with Tycho-2 9835 out of 13915 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits:
Forced-photometry filter: calibrated wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits -> calib.txt_param_ref_wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits (aperture=5.9)
Read 16789 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.5071 to 301.7244 deg, Dec -23.5973 to -12.1017 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 284.5071 to 301.7244 deg, Dec -23.5973 to -12.1017 deg
Loaded 14832 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): 10200 out of 10680 total matches.
Matched with Tycho-2 10680 out of 16789 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits:
Forced-photometry filter: calibrated wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits -> calib.txt_param_ref_wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
2.4 pix Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
2.6 pix fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
2.5 pix fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
2.1 pix wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
2.4 pix wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
Limiting magnitude estimates:
14.5 mag. Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
14.7 mag. Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
13.5 mag. fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
13.6 mag. fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2B5dxYuKEd (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_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1096, passed=13915
Got 13915 stars (including 12796 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat
util/solve_plate_with_UCAC5 got 13915 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 963 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13425 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 -12.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13425 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13425 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 960 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_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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.3uPdbOE4ZR (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_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1153, passed=16789
Got 16789 stars (including 15625 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat
util/solve_plate_with_UCAC5 got 16789 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
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(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 16191 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
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: 960 matched stars entering correct_measured_positions(), 16191 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 16191 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 960 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_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits -region wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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.Zvvt90DSDJ (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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.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_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=422, passed=5613
Got 5613 stars (including 5188 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat
util/solve_plate_with_UCAC5 got 5613 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5467 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5468 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 5467 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.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.8BhtIQL4iU (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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.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_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=473, passed=5518
Got 5518 stars (including 5041 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat
util/solve_plate_with_UCAC5 got 5518 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 5356 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 -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 5356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 5355 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 954 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.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_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits'
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:24:51.12 -14:37:57.8: 10.27 +/- 0.00 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:36:43.31 -18:43:51.7: 13.72 +/- 0.09 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:24:51.12 -14:37:57.8: 10.27 +/- 0.00 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:36:43.31 -18:43:51.7: 13.50 +/- 0.07 detection
Forced photometry reference-image weighted average: 10.27 +/- 0.00
Forced photometry filter REJECTED candidate at 19:24:51.12 -14:37:57.8: ref_mag=10.27 +/- 0.00 new_mean_mag=10.4415 delta=-0.17 (need > 0.90)
Forced photometry reference-image weighted average: 13.57 +/- 0.05
Forced photometry filter KEPT candidate at 19:36:43.31 -18:43:51.7: ref_mag=13.57 +/- 0.05 new_mean_mag=10.5884 delta=2.99 (need > 0.90)
Adding exclusion_list_local.txt__out23183.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: 1s
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Considering the candidate 23180_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 23180_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 23183_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
Preparing report for the candidate 23183_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
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 ####
19:36:43.31 -18:43:51.7
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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits exists and is non-empty
wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits (1st reference image)
verification OK: wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
Image size: 942.0'x627.4' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:19.463 -17:59:59.67 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits (1st new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 938.6'x624.7' 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: 19:33:41.779 -17:56:57.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:19.463 -17:59:59.67
Second-epoch image center 19:33:41.779 -17:56:57.34
Angular distance between the image centers 0.1019 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits (2nd new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 938.6'x624.7' 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: 19:33:42.386 -17:57:02.58 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:19.463 -17:59:59.67
Second-epoch image center 19:33:42.386 -17:57:02.58
Angular distance between the image centers 0.1033 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 19:33:41.779 -17:56:57.34
Second-epoch second image center 19:33:42.386 -17:57:02.58
Angular distance between the image centers 0.00281 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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits &> /tmp/tmp.o62xwtFWuG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits &> /tmp/tmp.QkGsPWzZVB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits &> /tmp/tmp.pqCaJHxWgW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits &> /tmp/tmp.pAH2pXrtsk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits and wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits and wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits and wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat' -> 'wcsmag.cat'
Read 136066 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7492 to 301.8063 deg, Dec -23.3001 to -12.5266 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 284.7492 to 301.8063 deg, Dec -23.3001 to -12.5266 deg
Loaded 13811 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): 9890 out of 12176 total matches.
Matched with Tycho-2 12176 out of 136066 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.622850
a=0.000000 b=1.000000 c=22.622850
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.67
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.67
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 136066 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7492 to 301.8063 deg, Dec -23.3001 to -12.5266 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 284.7492 to 301.8063 deg, Dec -23.3001 to -12.5266 deg
Loaded 13811 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): 9890 out of 12176 total matches.
Matched with Tycho-2 12176 out of 136066 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits:
Forced-photometry filter: calibrated wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits -> calib.txt_param_ref_wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits (aperture=4.4)
Read 143999 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.4734 to 301.7339 deg, Dec -23.5973 to -12.0912 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 284.4734 to 301.7339 deg, Dec -23.5973 to -12.0912 deg
Loaded 14871 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): 9826 out of 12171 total matches.
Matched with Tycho-2 12171 out of 143999 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits:
Forced-photometry filter: calibrated wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits -> calib.txt_param_ref_wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 45 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
2.3 pix Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
2.4 pix fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
2.2 pix fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
2.0 pix wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
2.3 pix wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
Limiting magnitude estimates:
14.7 mag. Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
14.8 mag. Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
13.7 mag. fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
13.7 mag. fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.1 (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.o62xwtFWuG (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_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_06-38-45_20.00sec_-15.00C_LIGHT_0389.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_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=12676, passed=136060
Got 136060 stars (including 123151 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat
util/solve_plate_with_UCAC5 got 136060 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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 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: 962 matched stars entering correct_measured_positions(), 939 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(), 132887 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 -12.5)
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: 961 matched stars entering correct_measured_positions(), 132884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 132884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 961 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_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.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.QkGsPWzZVB (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_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=14059, passed=143984
Got 143984 stars (including 129693 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat
util/solve_plate_with_UCAC5 got 143984 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
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: 964 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 139763 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 332 to 391 (Dec -23.6 to -12.1)
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: 964 matched stars entering correct_measured_positions(), 139762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 139761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits -region wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.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.pqCaJHxWgW (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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.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_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2706, passed=57172
Got 57172 stars (including 54387 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat
util/solve_plate_with_UCAC5 got 57172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 55745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 55750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 55750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 960 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_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.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.pAH2pXrtsk (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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.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_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2988, passed=61362
Got 61362 stars (including 58278 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat
util/solve_plate_with_UCAC5 got 61362 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 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(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 59453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 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: 960 matched stars entering correct_measured_positions(), 59453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 59453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 960 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_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.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_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-20-38_20.00sec_-5.00C_LIGHT_0302.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.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_2026-05-03_CI_Sgr-03-Q2b1x1_032205_TTUQ2b1x1_4034801_dfMxIMcG/wcs_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303.fits
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:39:17.62 -20:36:59.6: 13.28 +/- 0.06 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:49:39.45 -14:03:48.3: 12.76 +/- 0.03 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:17:51.32 -19:03:19.6: 12.63 +/- 0.03 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:47:42.10 -13:35:42.3: 13.01 +/- 0.04 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:46:22.80 -15:07:03.0: 12.84 +/- 0.04 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:17:26.86 -18:39:18.4: 12.76 +/- 0.05 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:49:59.63 -14:39:03.8: 13.15 +/- 0.05 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:49:14.00 -21:03:24.7: 12.46 +/- 0.03 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:12:17.90 -22:04:32.4: 12.53 +/- 0.04 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:49:39.45 -14:03:48.3: 12.81 +/- 0.03 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:47:42.10 -13:35:42.3: 13.02 +/- 0.04 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:46:22.80 -15:07:03.0: 12.76 +/- 0.03 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:39:17.62 -20:36:59.6: 13.24 +/- 0.05 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:49:59.63 -14:39:03.8: 13.11 +/- 0.04 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:17:26.86 -18:39:18.4: 12.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:17:51.32 -19:03:19.6: 12.57 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 19:49:39.45 -14:03:48.3: ref_mag=12.78 +/- 0.02 new_mean_mag=12.7660 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.01 +/- 0.03
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Forced photometry filter REJECTED candidate at 19:47:42.10 -13:35:42.3: ref_mag=13.01 +/- 0.03 new_mean_mag=12.8175 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:46:22.80 -15:07:03.0: ref_mag=12.79 +/- 0.02 new_mean_mag=12.8764 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.26 +/- 0.04
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Forced photometry reference-image weighted average: 12.70 +/- 0.03
Forced photometry filter REJECTED candidate at 19:49:59.63 -14:39:03.8: ref_mag=13.13 +/- 0.03 new_mean_mag=13.0506 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:39:17.62 -20:36:59.6: ref_mag=13.26 +/- 0.04 new_mean_mag=13.4871 delta=-0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:17:26.86 -18:39:18.4: ref_mag=12.70 +/- 0.03 new_mean_mag=12.8827 delta=-0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:17:51.32 -19:03:19.6: ref_mag=12.60 +/- 0.02 new_mean_mag=12.8439 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:49:14.00 -21:03:24.7: 12.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.02
Forced photometry filter REJECTED candidate at 19:49:14.00 -21:03:24.7: ref_mag=12.41 +/- 0.02 new_mean_mag=12.6615 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:12:17.90 -22:04:32.4: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Forced photometry filter REJECTED candidate at 19:12:17.90 -22:04:32.4: ref_mag=12.50 +/- 0.02 new_mean_mag=12.4385 delta=0.06 (need > 0.90)
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:08:33.76 -22:09:33.6: 11.43 +/- 0.01 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:33:34.74 -14:51:48.6: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:23:12.66 -21:32:49.7: 11.24 +/- 0.01 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:04:30.14 -21:49:29.7: 12.25 +/- 0.03 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:23:07.67 -18:59:42.5: 12.74 +/- 0.04 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:33:34.74 -14:51:48.6: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:08:33.76 -22:09:33.6: 11.43 +/- 0.01 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:23:12.66 -21:32:49.7: 11.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.01
Forced photometry filter REJECTED candidate at 19:08:33.76 -22:09:33.6: ref_mag=11.43 +/- 0.01 new_mean_mag=11.4604 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:04:30.14 -21:49:29.7: 11.96 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 19:23:12.66 -21:32:49.7: ref_mag=11.20 +/- 0.01 new_mean_mag=11.1809 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.06 +/- 0.02
Forced photometry filter REJECTED candidate at 19:04:30.14 -21:49:29.7: ref_mag=12.06 +/- 0.02 new_mean_mag=12.0052 delta=0.05 (need > 0.90)
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:14:50.87 -20:02:40.4: 12.64 +/- 0.04 detection
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:23:07.67 -18:59:42.5: 12.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.03
Forced photometry filter REJECTED candidate at 19:23:07.67 -18:59:42.5: ref_mag=12.77 +/- 0.03 new_mean_mag=12.6309 delta=0.14 (need > 0.90)
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:14:50.87 -20:02:40.4: 12.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.03
Forced photometry filter REJECTED candidate at 19:14:50.87 -20:02:40.4: ref_mag=12.66 +/- 0.03 new_mean_mag=12.6553 delta=0.01 (need > 0.90)
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-03-22_06-38-45_20.00sec_-15.00C_LIGHT_0389.fits at 19:50:49.31 -16:39:49.0: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q2b1x1_2026-04-16_05-37-49_20.00sec_-5.00C_LIGHTs_0363.fits at 19:50:49.31 -16:39:49.0: 15.47 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out164787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165102.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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
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Considering the candidate 164620_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164620_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164626_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164626_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:16:00.68 -14:50:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164630_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164630_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:50:38.17 -14:21:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164636_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164636_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:22:52.61 -18:00:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164640_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164640_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164644_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164644_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164648_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164648_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164649_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164649_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 164652_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164652_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 164655_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164655_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 164659_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164659_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:11:13.13 -22:06:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164664_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164664_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 164669_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164669_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 164671_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164671_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:30:54.98 -21:25:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164676_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164676_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:15:18.04 -14:07:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164678_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164678_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 164679_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164679_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:15:58.98 -14:26:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164680_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164680_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 164772_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164772_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 164787_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
Preparing report for the candidate 164787_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
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Considering the candidate 164796_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164796_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 164802_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164802_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:31:00.20 -21:18:28.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 164836_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164836_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:08:52.27 -18:57:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164842_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164842_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:36:26.30 -18:52:31.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 164845_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164845_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:26:26.81 -21:46:07.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 164855_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164855_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:35:39.88 -20:46:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164859_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164859_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:17:36.75 -15:57:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164866_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164866_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:18:07.56 -18:52:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164871_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164871_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 164879_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164879_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:34:17.97 -16:20:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164907_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164907_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
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Considering the candidate 164908_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164908_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:17:24.71 -20:43:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164925_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164925_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:19:04.92 -15:55:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164946_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164946_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:40:49.23 -16:18:28.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 164947_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164947_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:18:52.47 -19:43:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164951_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164951_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:26:21.63 -21:14:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164954_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164954_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:19:03.24 -15:55:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164955_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164955_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:13:01.01 -20:12:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164961_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164961_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:51:10.34 -15:10:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164979_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 164979_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 165004_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 165004_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 165013_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 165013_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:26:42.88 -16:47:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165102_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
Preparing report for the candidate 165102_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
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Considering the candidate 53345_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 53345_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks
**** FOUND 19:36:43.30 -18:43:51.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 109826_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303
The candidate 109826_fd_Sgr-03-Q2b1x1_2026-05-03_03-21-22_20.00sec_-5.00C_LIGHT_0303 did not pass the final checks