This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 25.1011 2461155.6011 11.93 05:16:06.88 +25:56:50.9
178.91903 -7.11296 galactic Tau Second-epoch detections are separated by 1.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.471 Papagena 1 0 1 11.6 -0 -0
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:16:06.88 +25:56:50.9: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:16:06.88 +25:56:50.9: 16.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 25.1011* 05 16 06.88 +25 56 50.9 11.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461155.6011,11.93,0.05,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 20260425.1011 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1011 2461155.6011 12.70 05:09:28.94 +27:53:34.0
176.45787 -7.19126 galactic Tau Second-epoch detections are separated by 1.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.68 Leto 2 -0 2 12.7 -0 -0
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:09:28.94 +27:53:34.0: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:09:28.94 +27:53:34.0: 16.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 25.1011* 05 09 28.94 +27 53 34.0 12.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461155.6011,12.70,0.05,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 20260425.1011 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1011 2461155.6011 13.33 04:51:58.58 +28:15:44.8
173.80137 -10.04585 galactic Tau Second-epoch detections are separated by 6.5" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:51:58.58 +28:15:44.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:51:58.58 +28:15:44.8: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:51:58.58 +28:15:44.8: 16.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 25.1011* 04 51 58.58 +28 15 44.8 13.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461155.6011,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260425.1011 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1011 2461155.6011 13.77 05:15:15.76 +29:53:13.0
175.56917 -5.00119 galactic Aur Second-epoch detections are separated by 1.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.925 Alphonsina 2 -0 2 13.9 -0 0
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:15:15.76 +29:53:13.0: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:15:15.76 +29:53:13.0: 16.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461155.6011,13.77,0.05,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 20260425.1011 13.77CV 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: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461155.60136186 25.04.2026 02:25:47.665 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
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): 12752
Objects passed selection criteria: 12681
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 8816.75
Average stars matched: 8551.5 (96.9915 %)
Memory usage VmPeak: 118868 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 24 21:28:34 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: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461155.60136186 25.04.2026 02:25:47.665 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 68
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.26
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: 21 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): 101389
Objects passed selection criteria: 101163
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 74568
Average stars matched: 71464 (95.8374 %)
Memory usage VmPeak: 1939140 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 24 21:30:53 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.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: 2461155.60082755
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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
Saving wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits to local_wcs_cache/
'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
Saving wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits to local_wcs_cache/
'wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits'
wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (1st reference image)
verification OK: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:01.017 +29:59:40.48 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits (1st new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:00:00.610 +30:00:11.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:01.017 +29:59:40.48
Second-epoch image center 05:00:00.610 +30:00:11.12
Angular distance between the image centers 0.0086 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits (2nd new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:00:02.146 +30:00:05.32 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:01.017 +29:59:40.48
Second-epoch image center 05:00:02.146 +30:00:05.32
Angular distance between the image centers 0.0080 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 05:00:00.610 +30:00:11.12
Second-epoch second image center 05:00:02.146 +30:00:05.32
Angular distance between the image centers 0.00577 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.yperzDjb1o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.V1tAa6lRzQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits &> /tmp/tmp.sSiUQgcAmP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits &> /tmp/tmp.0l66GVfr2W
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
The reference image (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat) found
'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat' -> 'wcsmag.cat'
Read 16295 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5643 to 84.6645 deg, Dec +24.3655 to +35.2867 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 65.5643 to 84.6645 deg, Dec 24.3655 to 35.2867 deg
Loaded 8424 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): 6043 out of 6742 total matches.
Matched with Tycho-2 6742 out of 16295 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.979657
a=0.000000 b=1.000000 c=22.979657
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 16295 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5643 to 84.6645 deg, Dec +24.3655 to +35.2867 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 65.5643 to 84.6645 deg, Dec 24.3655 to 35.2867 deg
Loaded 8424 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): 6043 out of 6742 total matches.
Matched with Tycho-2 6742 out of 16295 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -> calib.txt_param_ref_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (aperture=5.9)
Read 16349 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5645 to 84.6680 deg, Dec +24.3653 to +35.2868 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 65.5645 to 84.6680 deg, Dec 24.3653 to 35.2868 deg
Loaded 8428 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): 6047 out of 6745 total matches.
Matched with Tycho-2 6745 out of 16349 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -> calib.txt_param_ref_wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.6 pix fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
2.6 pix fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
1.9 pix wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Limiting magnitude estimates:
15.4 mag. Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.4 mag. Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
13.9 mag. fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
13.8 mag. fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.1 (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.yperzDjb1o (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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1498, passed=16295
Got 16295 stars (including 14768 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
util/solve_plate_with_UCAC5 got 16295 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15808 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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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.V1tAa6lRzQ (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/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1486, passed=16349
Got 16349 stars (including 14839 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat
util/solve_plate_with_UCAC5 got 16349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.sSiUQgcAmP (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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=408, passed=4878
Got 4878 stars (including 4468 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 4878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits -region wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.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.0l66GVfr2W (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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=421, passed=4728
Got 4728 stars (including 4304 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 4728 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 4572 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 4577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 4577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits -region wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits'
Preparing the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Creating symlink local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (1st reference image)
verification OK: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:01.017 +29:59:40.48 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits (1st new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:00:00.610 +30:00:11.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:01.017 +29:59:40.48
Second-epoch image center 05:00:00.610 +30:00:11.12
Angular distance between the image centers 0.0086 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits (2nd new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:00:02.146 +30:00:05.32 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:01.017 +29:59:40.48
Second-epoch image center 05:00:02.146 +30:00:05.32
Angular distance between the image centers 0.0080 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 05:00:00.610 +30:00:11.12
Second-epoch second image center 05:00:02.146 +30:00:05.32
Angular distance between the image centers 0.00577 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.5RPv1lxc0i
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.k8DTA67NTL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits &> /tmp/tmp.dnVHm9GGQC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits &> /tmp/tmp.jHR528Mf8J
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
The reference image (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat) found
'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat' -> 'wcsmag.cat'
Read 129003 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5568 to 84.6878 deg, Dec +24.3237 to +35.3004 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 65.5568 to 84.6878 deg, Dec 24.3237 to 35.3004 deg
Loaded 8482 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): 4945 out of 6875 total matches.
Matched with Tycho-2 6875 out of 129003 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.825003
a=0.000000 b=1.000000 c=22.825003
From vast_summary.log: estimated ref. image limiting mag.: -7.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 129003 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5568 to 84.6878 deg, Dec +24.3237 to +35.3004 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 65.5568 to 84.6878 deg, Dec 24.3237 to 35.3004 deg
Loaded 8482 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): 4945 out of 6875 total matches.
Matched with Tycho-2 6875 out of 129003 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -> calib.txt_param_ref_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (aperture=4.4)
Read 129055 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5645 to 84.6893 deg, Dec +24.3196 to +35.2959 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 65.5645 to 84.6893 deg, Dec 24.3196 to 35.2959 deg
Loaded 8478 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): 4939 out of 6881 total matches.
Matched with Tycho-2 6881 out of 129055 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -> calib.txt_param_ref_wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 49 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.8 pix Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.4 pix fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
2.3 pix fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
1.8 pix wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Limiting magnitude estimates:
15.6 mag. Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.6 mag. Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
14.1 mag. fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
14.1 mag. fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.5 (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.5RPv1lxc0i (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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=14027, passed=128967
Got 128967 stars (including 114720 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
util/solve_plate_with_UCAC5 got 128967 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 125973 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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 125971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 125971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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.k8DTA67NTL (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/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=13827, passed=129020
Got 129020 stars (including 114972 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat
util/solve_plate_with_UCAC5 got 129020 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 126156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 126161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 126159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dnVHm9GGQC (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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2939, passed=42712
Got 42712 stars (including 39715 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 42712 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 41483 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 41483 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 41483 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits -region wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.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.jHR528Mf8J (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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2270, passed=41742
Got 41742 stars (including 39424 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 41742 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 40895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 40895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 40894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits -region wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-01_20.00sec_-5.00C_LIGHT_0011.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.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_2026-04-24_CI_Aur-05-Q2b1x1_212625_TTUQ2b1x1_2912249_MZDVOny2/wcs_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012.fits
Preparing the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out149704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out149936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151120.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 149704_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149704_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:59:06.91 +27:36:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.578 154119786112974336 074.77894383962 +27.60155922800 13.5474 12.7548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149723_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149723_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:29:32.44 +33:28:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.209 3449146226622055168 082.38521327866 +33.47505588781 13.2386 12.4456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149730_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149730_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:21:23.87 +27:39:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.967 3421484683024723456 080.35007340368 +27.65554140093 12.8535 12.4216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149732_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149732_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:48:16.55 +27:54:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149869_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149869_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 149888_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149888_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:56:57.84 +33:05:59.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 149908_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149908_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:41:14.09 +28:37:41.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 149926_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149926_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:18:17.94 +33:47:33.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 149936_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
Preparing report for the candidate 149936_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
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Considering the candidate 149941_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149941_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:22:15.64 +26:10:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149956_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149956_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:55:45.14 +30:20:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149975_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149975_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:56:56.90 +33:06:50.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 149982_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149982_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 149999_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 149999_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:15:29.68 +32:42:36.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 150025_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150025_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:27:57.01 +33:47:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150047_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150047_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:26:33.03 +28:37:19.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 150049_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150049_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:14:46.47 +31:23:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.230 180472502851498368 078.69389400240 +31.39758644300 12.4452 11.7561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150102_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150102_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:21:11.40 +29:32:54.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 150169_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150169_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:05:45.94 +26:25:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150204_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150204_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:51:21.87 +28:31:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150235_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
Preparing report for the candidate 150235_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
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Considering the candidate 150329_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150329_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:26:45.74 +30:29:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150387_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150387_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:18:28.38 +33:11:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150426_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150426_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:20:06.55 +32:46:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150521_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150521_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:01:54.50 +28:18:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.435 155668001564070144 075.47668014788 +28.30443136604 13.2401 12.7305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150632_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150632_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:05:16.12 +32:38:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.705 181625512592072320 076.31728166219 +32.63725356580 13.0955 12.3155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150660_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150660_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:59:17.64 +32:33:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150714_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150714_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:22:00.52 +32:53:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150737_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150737_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:09:49.66 +29:48:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150756_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150756_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:12:52.67 +32:19:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.033 181419903917075968 078.21921225062 +32.33142010630 13.6257 13.1004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150774_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
Preparing report for the candidate 150774_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
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Considering the candidate 150834_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150834_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:04:49.95 +29:58:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.415 156309218704622336 076.20824897290 +29.97637446617 13.2663 12.6748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150873_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150873_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:24:36.51 +30:33:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150878_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150878_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:48:17.57 +29:45:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150893_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150893_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 150967_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150967_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:01:47.88 +32:14:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150979_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 150979_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 151083_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 151083_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:10:31.73 +30:49:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151094_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 151094_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:15:53.18 +30:28:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151120_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
Preparing report for the candidate 151120_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
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Considering the candidate 151148_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 151148_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 151159_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 151159_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:49:22.14 +29:33:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151165_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 151165_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 04:58:15.27 +30:17:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143449_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 143449_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:10:32.19 +32:10:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76531_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 76531_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:16:37.56 +29:52:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16878_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 16878_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:10:41.87 +33:57:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105568_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 105568_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:15:47.36 +26:45:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139913_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 139913_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks
**** FOUND 05:26:52.99 +30:33:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62859_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012
The candidate 62859_fd_Aur-05-Q2b1x1_2026-04-24_21-25-47_20.00sec_-4.90C_LIGHT_0012 did not pass the final checks