This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3055859683398334336,2461133.6181,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3055859683398334336 20260403.1181 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461133.6181,12.60,0.05,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
target 20260403.1181 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461133.6181,12.01,0.05,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
target 20260403.1181 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0725233-075609,2461133.6181,11.51,0.05,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
NSVS J0725233-075609 20260403.1181 11.51CV 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: 2461119.60652544 20.03.2026 02:33:13.798 /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
First image: 2461119.60652544 20.03.2026 02:33:13.798 /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
Last image: 2461133.61837138 03.04.2026 02:50:17.287 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.08
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): 24044
Objects passed selection criteria: 23842
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 13859.5
Average stars matched: 13339.8 (96.2499 %)
Memory usage VmPeak: 128912 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 2 15:05:05 CDT 2026
VaST build number 1.0rc88-377-g075272b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 21:56:01 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: 2461119.60652544 20.03.2026 02:33:13.798 /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
First image: 2461119.60652544 20.03.2026 02:33:13.798 /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
Last image: 2461133.61837138 03.04.2026 02:50:17.287 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 54
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
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: 30 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): 172690
Objects passed selection criteria: 172011
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 106827
Average stars matched: 101406 (94.9257 %)
Memory usage VmPeak: 2065608 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 2 15:05:05 CDT 2026
VaST build number 1.0rc88-377-g075272b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 22:00:18 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/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
SExtractor catalog cache: saved Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
SExtractor catalog cache: saved Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.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/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.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: 2461133.61778293
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
Saving wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits'
wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
Saving wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits to local_wcs_cache/
'wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits'
wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits exists and is non-empty
Saving wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits to local_wcs_cache/
'wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits' -> 'local_wcs_cache/wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits'
wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits exists and is non-empty
Saving wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits to local_wcs_cache/
'wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits' -> 'local_wcs_cache/wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:42:46.255 -09:59:55.21
Second-epoch image center 07:42:52.597 -09:59:53.47
Angular distance between the image centers 0.0260 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:42:46.255 -09:59:55.21
Second-epoch image center 07:42:52.960 -09:59:47.76
Angular distance between the image centers 0.0276 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 07:42:52.597 -09:59:53.47
Second-epoch second image center 07:42:52.960 -09:59:47.76
Angular distance between the image centers 0.00218 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/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.ob2ftZS4FR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.2SyRYfKLVU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits &> /tmp/tmp.7uZr1Kcfg7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits &> /tmp/tmp.5mQd5v9XtB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.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_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits and wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.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_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits and wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat
Found non-empty wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits and wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat
The reference image (wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits) and catalog (wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat) found
'wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat' -> 'wcsmag.cat'
Read 29086 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 107.5371 to 123.6872 deg, Dec -15.2912 to -4.5931 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 107.5371 to 123.6872 deg, Dec -15.2912 to -4.5931 deg
Loaded 24807 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): 16796 out of 18331 total matches.
Matched with Tycho-2 18331 out of 29086 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.871895
a=0.000000 b=1.000000 c=22.871895
From vast_summary.log: estimated ref. image limiting mag.: -8.08
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.79
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.79
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
2.5 pix Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
2.5 pix fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
2.6 pix fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
Limiting magnitude estimates:
14.8 mag. Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
14.8 mag. Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
11.7 mag. fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
11.9 mag. fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
All-image limiting magnitude estimate: 11.7 (SNR ) 9.7 (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.ob2ftZS4FR (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2950, passed=29086
Got 29086 stars (including 26116 good ones) from the SExtractor catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 29086 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 949 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.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.2SyRYfKLVU (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2922, passed=28978
Got 28978 stars (including 26039 good ones) from the SExtractor catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 28978 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.75"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.75"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 949 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.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.7uZr1Kcfg7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=147, passed=2674
Got 2674 stars (including 2527 good ones) from the SExtractor catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 2674 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.71"
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits -region wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.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.5mQd5v9XtB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
WCS-calibrated image found: wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
Checking if the catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
WCS catalog name: wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=154, passed=2882
Got 2882 stars (including 2727 good ones) from the SExtractor catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 2882 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.72"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.74"
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits -region wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.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_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits'
Saving fully-calibrated image wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits'
Saving fully-calibrated image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits'
Saving fully-calibrated image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits'
Preparing the HTML report for the field Mon-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31697_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 31697_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 08:06:26.40 -09:14:14.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Mon-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
SExtractor catalog cache: saved Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
SExtractor catalog cache: saved Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.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_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits exists and is non-empty
wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:42:46.255 -09:59:55.21
Second-epoch image center 07:42:52.597 -09:59:53.47
Angular distance between the image centers 0.0260 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:42:46.255 -09:59:55.21
Second-epoch image center 07:42:52.960 -09:59:47.76
Angular distance between the image centers 0.0276 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 07:42:52.597 -09:59:53.47
Second-epoch second image center 07:42:52.960 -09:59:47.76
Angular distance between the image centers 0.00218 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/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.8oNyTSxUWn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.rxbwGCc6Tq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits &> /tmp/tmp.0cWCEhpxvL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits &> /tmp/tmp.CeneRFoypk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.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_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits and wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.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_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits and wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat
Found non-empty wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits and wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat
The reference image (wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits) and catalog (wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat) found
'wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat' -> 'wcsmag.cat'
Read 203060 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 107.5165 to 123.6907 deg, Dec -15.2923 to -4.5813 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 107.5165 to 123.6907 deg, Dec -15.2923 to -4.5813 deg
Loaded 24871 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): 14449 out of 20775 total matches.
Matched with Tycho-2 20775 out of 203060 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.677319
a=0.000000 b=1.000000 c=22.677319
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.94
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.94
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 28 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
2.3 pix Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
2.3 pix fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
2.4 pix fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
Limiting magnitude estimates:
14.9 mag. Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
14.9 mag. Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
12.3 mag. fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
12.4 mag. fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
All-image limiting magnitude estimate: 12.3 (SNR ) 12.0 (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.8oNyTSxUWn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=54, blended=31232, passed=203006
Got 203006 stars (including 171558 good ones) from the SExtractor catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 203006 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.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.rxbwGCc6Tq (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=62, blended=31956, passed=205869
Got 205869 stars (including 173699 good ones) from the SExtractor catalog wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 205869 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.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.0cWCEhpxvL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1141, passed=30178
Got 30178 stars (including 28993 good ones) from the SExtractor catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 30178 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits -region wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.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.CeneRFoypk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
WCS-calibrated image found: wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
Checking if the catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
WCS catalog name: wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1352, passed=31752
Got 31752 stars (including 30355 good ones) from the SExtractor catalog wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 31752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits -region wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.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_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/wcs_Mon-06-Q2b1x1_2026-03-19_21-33-13_20.00sec_-14.90C_LIGHT_0042.fits
Saving fully-calibrated image wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/wcs_Mon-06-Q2b1x1_2026-03-19_21-34-00_20.00sec_-15.00C_LIGHT_0043.fits
Saving fully-calibrated image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-49-26_20.00sec_-5.00C_LIGHT_0013.fits
Saving fully-calibrated image wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Mon-06-Q2b1x1_215102_TTUQ2b1x1_24210_iA4VREdQ/wcs_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014.fits
Preparing the HTML report for the field Mon-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out230998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out231007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out147777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out233851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55445.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 230998_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 230998_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:38:21.34 -08:15:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.597 3042007653654593792 114.58924384165 -08.26144226334 12.6100 12.1827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 231006_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 231006_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:38:04.45 -05:44:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231007_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 231007_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:44:32.65 -11:35:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 1.760 3036967840249100928 116.13609690430 -11.60040252657 10.8327 9.8029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 231010_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 231010_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:59:03.61 -09:31:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231018_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 231018_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:36:31.75 -06:20:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231020_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 231020_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 08:00:31.39 -13:54:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231021_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 231021_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:57:10.24 -13:23:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231776_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 231776_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 231938_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 231938_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 232905_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 232905_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 233851_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
Preparing report for the candidate 233851_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
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Considering the candidate 233875_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 233875_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:45:57.03 -06:43:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233902_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 233902_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:29:26.90 -07:34:44.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 234015_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 234015_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:37:23.39 -12:06:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.209 3033952773210378240 114.34770961044 -12.10699340748 11.8284 11.6652 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234076_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 234076_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:32:01.10 -08:53:33.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 234117_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 234117_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 234171_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 234171_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:40:41.13 -08:12:00.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 234269_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 234269_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:31:54.92 -08:40:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.635 3053604310173045504 112.97848694249 -08.67202074899 12.5554 12.3274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234327_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 234327_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:42:33.39 -06:14:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234420_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
Preparing report for the candidate 234420_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
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Considering the candidate 29363_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 29363_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:51:46.14 -13:53:60.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 55445_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
Preparing report for the candidate 55445_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
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Considering the candidate 190186_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 190186_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 147777_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
Preparing report for the candidate 147777_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
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Considering the candidate 121256_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 121256_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:41:14.73 -09:33:05.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 63948_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 63948_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:47:56.47 -12:11:29.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 114485_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 114485_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks
**** FOUND 07:30:47.69 -09:46:35.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 28715_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014
The candidate 28715_fd_Mon-06-Q2b1x1_2026-04-02_21-50-17_20.00sec_-4.90C_LIGHT_0014 did not pass the final checks