This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ
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 3525230992448096896,2461138.8146,11.78,0.05,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 3525230992448096896 20260408.3146 11.78CV 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
VARIABLE_NAME,2461138.8146,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260408.3146 12.26CV 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
VARIABLE_NAME,2461138.8146,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260408.3146 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
RU Crv,2461138.8146,7.88,0.05,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
RU Crv 20260408.3146 7.88CV 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
ASAS J122412-1930.1,2461138.8146,11.12,0.05,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
ASAS J122412-1930.1 20260408.3146 11.12CV 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
WX Crv,2461138.8146,10.13,0.05,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
WX Crv 20260408.3146 10.13CV 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: 2461082.92034660 11.02.2026 10:05:07.946 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
First image: 2461082.92034660 11.02.2026 10:05:07.946 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Last image: 2461138.81488207 08.04.2026 07:33:15.811 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 69
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.93
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): 4441
Objects passed selection criteria: 4434
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 4109.75
Average stars matched: 4011.5 (97.6093 %)
Memory usage VmPeak: 110808 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 02:35:18 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: 2461082.92034660 11.02.2026 10:05:07.946 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
First image: 2461082.92034660 11.02.2026 10:05:07.946 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Last image: 2461138.81488207 08.04.2026 07:33:15.811 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 78
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 28489
Objects passed selection criteria: 28415
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 23801
Average stars matched: 23145.8 (97.247 %)
Memory usage VmPeak: 134372 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 02:36:11 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/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
SExtractor catalog cache: saved Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat to cache
SExtractor catalog cache: saved Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.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/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.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: 2461138.81435094
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_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits exists and is non-empty
Saving wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits to local_wcs_cache/
'wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits' -> 'local_wcs_cache/wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits'
wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
Saving wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits to local_wcs_cache/
'wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits' -> 'local_wcs_cache/wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits'
wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits exists and is non-empty
Saving wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits to local_wcs_cache/
'wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits' -> 'local_wcs_cache/wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits'
wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits exists and is non-empty
Saving wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits to local_wcs_cache/
'wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits' -> 'local_wcs_cache/wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:26:39.749 -18:00:06.86
Second-epoch image center 12:26:41.734 -18:00:46.27
Angular distance between the image centers 0.0135 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 12:26:39.749 -18:00:06.86
Second-epoch image center 12:26:39.911 -18:00:48.84
Angular distance between the image centers 0.0117 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 12:26:41.734 -18:00:46.27
Second-epoch second image center 12:26:39.911 -18:00:48.84
Angular distance between the image centers 0.00726 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/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits &> /tmp/tmp.QIzbMseaFZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.skgKZvZ1mU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits &> /tmp/tmp.PnN3pVjxnI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits &> /tmp/tmp.4Y8DFO6Fj7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
Calibrating the magnitude scale
Found non-empty wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
Found non-empty wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
The reference image (wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits) and catalog (wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat) found
'wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat' -> 'wcsmag.cat'
Read 5826 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.3232 to 195.2856 deg, Dec -23.3230 to -12.5315 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 178.3232 to 195.2856 deg, Dec -23.3230 to -12.5315 deg
Loaded 5194 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): 3909 out of 4081 total matches.
Matched with Tycho-2 4081 out of 5826 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.822012
a=0.000000 b=1.000000 c=22.822012
From vast_summary.log: estimated ref. image limiting mag.: -7.93
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
2.1 pix Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
4.5 pix fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
4.5 pix fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
Limiting magnitude estimates:
14.9 mag. Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
14.9 mag. Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
13.9 mag. fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
13.9 mag. fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.6 (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.QIzbMseaFZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits' -> 'wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS-calibrated image found: wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Checking if the catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS catalog name: wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=465, passed=5826
Got 5826 stars (including 5355 good ones) from the SExtractor catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 5826 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5723 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits -region wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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.skgKZvZ1mU (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits' -> 'wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=457, passed=5792
Got 5792 stars (including 5328 good ones) from the SExtractor catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 5792 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.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.PnN3pVjxnI (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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
WCS_IMAGE_NAME=wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
WCS-calibrated image found: wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
Checking if the catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat corresponding to the image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits alredy exist and is non-empty...
Catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat corresponding to the image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
WCS catalog name: wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=596, passed=4673
Got 4673 stars (including 4076 good ones) from the SExtractor catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat
util/solve_plate_with_UCAC5 got 4673 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 972 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits -region wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.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.4Y8DFO6Fj7 (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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
WCS-calibrated image found: wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
Checking if the catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat corresponding to the image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat corresponding to the image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
WCS catalog name: wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=608, passed=4696
Got 4696 stars (including 4087 good ones) from the SExtractor catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat
util/solve_plate_with_UCAC5 got 4696 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4425 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4425 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 972 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits -region wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.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_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits'
Saving fully-calibrated image wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits'
Saving fully-calibrated image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits'
Saving fully-calibrated image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits'
Preparing the HTML report for the field Crv-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20202.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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 20189_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20189_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:19:38.05 -19:15:20.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20191_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20191_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:46:09.29 -14:49:07.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20193_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20193_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:53:50.81 -13:50:44.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20194_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20194_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:21:52.58 -13:53:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20196_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20196_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:54:33.02 -14:00:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.088 3525832012991427200 193.63731475568 -13.99987491457 12.0705 11.4106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20198_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20198_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:40:35.52 -17:05:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20199_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20199_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:54:22.95 -18:11:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 0.610 3510330750169788800 193.59547267843 -18.19778270727 11.9284 11.5016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20202_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
Preparing report for the candidate 20202_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
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Considering the candidate 20203_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20203_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:52:11.32 -15:26:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 0.480 3524453358553367040 193.04703195820 -15.44003010187 12.0409 11.5390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20207_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20207_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:45:05.30 -15:01:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 1.749 3524032352974713728 191.27164992785 -15.02869114568 12.0297 11.6817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20211_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20211_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:44:24.43 -17:30:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 0.375 3522323711905249536 191.10183948857 -17.51503800168 11.8208 11.1357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20213_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20213_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:51:30.91 -16:15:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.668 3522860204860320768 192.87860539566 -16.25729911642 12.0875 11.5558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20216_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20216_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:48:12.26 -20:16:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.912 3503512889020305664 192.05134089401 -20.27515986523 11.9069 11.1454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20218_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20218_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:45:07.01 -13:53:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 1.348 3528605118755524480 191.27957138335 -13.89440124639 11.8870 11.1106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20220_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20220_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:54:06.96 -17:43:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.357 3510503132977426944 193.52910107103 -17.72588431958 11.9880 11.3452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20222_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20222_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:43:02.71 -18:08:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 0.433 3522156620497680640 190.76117412518 -18.13532207218 11.9819 11.5472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20224_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20224_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:42:06.27 -17:35:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.569 3522987675194074880 190.52598574341 -17.58664148023 11.9883 11.5119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20225_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20225_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:39:51.72 -13:44:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 0.210 3527411598883647744 189.96552762584 -13.74739267198 12.0383 11.4739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20227_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20227_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:42:26.59 -16:13:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 0.757 3523787707341995136 190.61079663517 -16.22398787672 12.0241 11.6012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20229_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20229_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:50:59.08 -19:30:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 3.452 3509663312251986560 192.74717547622 -19.51084775393 12.2401 11.7446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20240_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20240_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:53:08.23 -14:39:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.225 3525364578814801280 193.28434223194 -14.65095553266 12.0582 11.4994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20241_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20241_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:55:10.39 -16:50:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 1.225 3522582676957932160 193.79294923319 -16.84503628107 12.1270 11.7043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20242_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20242_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:46:24.17 -20:10:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.250 3503703207611126528 191.60069375105 -20.17323744879 12.0630 11.6548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20243_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20243_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:43:22.44 -14:42:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.969 3527058788794668544 190.84340765234 -14.70128175132 12.1100 11.5787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20244_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20244_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:52:24.68 -15:49:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 0.673 3524422606587549568 193.10265642172 -15.82502189954 12.0740 11.5381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20247_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20247_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:47:11.80 -18:41:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.302 3521961422823986048 191.79925431997 -18.69290434894 12.0759 11.6076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20248_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20248_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:53:33.43 -18:21:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.858 3510304434906172544 193.38953164274 -18.36429236383 12.0488 11.3709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20251_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20251_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:49:31.43 -22:00:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 2.596 3502442785032647808 192.38103518460 -22.01572684390 12.1477 11.7449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20255_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20255_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:51:17.18 -21:30:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.642 3502586958495091200 192.82187526379 -21.50651264942 12.2763 11.6916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20258_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20258_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:52:47.62 -18:10:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.761 3510360402623999360 193.19819575797 -18.17664161178 12.1552 11.7056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20259_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20259_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:53:13.18 -20:54:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 0.648 3508617230017396864 193.30475021619 -20.90931314290 12.2222 11.7660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20260_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20260_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:52:00.67 -16:10:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 1.002 3522866767570447488 193.00252468420 -16.17838636080 12.1238 11.6080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20261_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20261_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:51:49.12 -18:24:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.504 3510349373147990784 192.95452266696 -18.40708669610 12.1228 11.6889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20263_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20263_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:49:42.93 -17:15:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.493 3522506436994071296 192.42874108604 -17.25554860428 12.1687 11.6616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20264_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20264_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:48:26.34 -17:54:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.082 3522075080543262976 192.10951963657 -17.90909446279 12.1659 11.8112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20265_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20265_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:48:55.24 -14:55:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 0.769 3525294691106983424 192.23004769023 -14.93192994650 12.0451 11.5118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02998_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 02998_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:35:01.98 -18:27:38.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 15s
Prepared the HTML report for the field Crv-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
12:52:36.52 -15:13:39.3
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/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
SExtractor catalog cache: saved Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat to cache
SExtractor catalog cache: saved Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Creating symlink local_wcs_cache/wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Creating symlink local_wcs_cache/wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
Creating symlink local_wcs_cache/wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.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_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits exists and is non-empty
wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits exists and is non-empty
wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:26:39.749 -18:00:06.86
Second-epoch image center 12:26:41.734 -18:00:46.27
Angular distance between the image centers 0.0135 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 12:26:39.749 -18:00:06.86
Second-epoch image center 12:26:39.911 -18:00:48.84
Angular distance between the image centers 0.0117 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 12:26:41.734 -18:00:46.27
Second-epoch second image center 12:26:39.911 -18:00:48.84
Angular distance between the image centers 0.00726 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/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits &> /tmp/tmp.E7p4CMJlk6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.RY39JoyWOi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits &> /tmp/tmp.I7C5mopJIr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits &> /tmp/tmp.f1FM5HcmrM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
Calibrating the magnitude scale
Found non-empty wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
Found non-empty wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
The reference image (wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits) and catalog (wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat) found
'wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat' -> 'wcsmag.cat'
Read 38658 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.2863 to 195.3102 deg, Dec -23.3302 to -12.4639 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 178.2863 to 195.3102 deg, Dec -23.3302 to -12.4639 deg
Loaded 5234 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): 4057 out of 4444 total matches.
Matched with Tycho-2 4444 out of 38658 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.659516
a=0.000000 b=1.000000 c=22.659516
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.06
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.06
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 20 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
1.9 pix Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
3.9 pix fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
3.9 pix fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
Limiting magnitude estimates:
15.1 mag. Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
15.0 mag. Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
14.3 mag. fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
14.4 mag. fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.E7p4CMJlk6 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits' -> 'wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS-calibrated image found: wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Checking if the catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS catalog name: wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1533, passed=38642
Got 38642 stars (including 37036 good ones) from the SExtractor catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 38642 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 38118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 38118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
WARNING: Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 38118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits -region wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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.RY39JoyWOi (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits' -> 'wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1495, passed=38320
Got 38320 stars (including 36755 good ones) from the SExtractor catalog wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 38320 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 37640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 37640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
WARNING: Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 37640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.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.I7C5mopJIr (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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
WCS_IMAGE_NAME=wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
WCS-calibrated image found: wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
Checking if the catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat corresponding to the image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits alredy exist and is non-empty...
Catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat corresponding to the image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
WCS catalog name: wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=2815, passed=20342
Got 20342 stars (including 17517 good ones) from the SExtractor catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat
util/solve_plate_with_UCAC5 got 20342 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 19217 with non-zero local correction accuracy
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 19218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 19218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits -region wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.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.f1FM5HcmrM (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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
WCS-calibrated image found: wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
Checking if the catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat corresponding to the image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat corresponding to the image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
WCS catalog name: wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2877, passed=20648
Got 20648 stars (including 17762 good ones) from the SExtractor catalog wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat
util/solve_plate_with_UCAC5 got 20648 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 19156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 19156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 19155 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits -region wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.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_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/wcs_Crv-01-Q2b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Saving fully-calibrated image wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/wcs_Crv-01-Q2b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Saving fully-calibrated image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-32-29_20.00sec_-4.90C_LIGHT_0136.fits
Saving fully-calibrated image wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.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_2026-04-08_CI_Crv-01-Q2b1x1_023406_TTUQ2b1x1_28583_JPxldkRJ/wcs_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137.fits
Preparing the HTML report for the field Crv-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out34082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52299.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 52208_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 52208_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:08:19.10 -13:56:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 5.069 3570509190517385472 182.08051359527 -13.93583031787 13.3983 12.9648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52215_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 52215_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:32:27.68 -20:57:28.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 52250_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 52250_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:10:23.89 -21:26:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 0.440 3517392020002225024 182.59950311540 -21.44545017667 12.4302 11.9366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52290_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
Preparing report for the candidate 52290_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
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Considering the candidate 52297_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 52297_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:40:32.17 -17:38:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52299_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
Preparing report for the candidate 52299_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
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Considering the candidate 52334_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 52334_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:36:47.61 -15:33:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34082_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
Preparing report for the candidate 34082_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
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Considering the candidate 38500_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
Preparing report for the candidate 38500_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
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Considering the candidate 20083_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 20083_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:35:01.93 -18:27:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34964_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
Preparing report for the candidate 34964_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
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Considering the candidate 28390_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 28390_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:19:38.03 -19:15:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03548_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 03548_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:21:52.57 -13:53:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12032_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 12032_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:29:51.24 -16:31:02.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 11031_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 11031_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:32:03.18 -16:11:50.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 12829_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 12829_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:17:03.24 -16:41:38.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 15652_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 15652_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:15:48.34 -17:32:30.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 34402_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 34402_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:14:59.66 -20:50:37.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 30021_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 30021_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks
**** FOUND 12:20:10.55 -22:10:32.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 29483_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137
The candidate 29483_fd_Crv-01-Q2b1x1_2026-04-08_02-33-15_20.00sec_-4.90C_LIGHT_0137 did not pass the final checks