This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te
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 08 22.3754 2461274.8754 9.70 18:23:56.52 +39:35:02.3
67.38986 21.87915 galactic Lyr Second-epoch detections are separated by 3.3" and 4.3 pix
The object was found in VSX 4" TW Lyr
Type: M
# Max. Min./Amp. JD0 Period
9.500 V 14.900 V 2443039.00000 376.710000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:23:56.52 +39:35:02.3: 10.76 +/- 0.00 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:23:56.52 +39:35:02.3: 10.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.00
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
TW Lyr,2461274.8754,9.70,0.05,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
TW Lyr 20260822.3754 9.70CV 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 08 22.3754 2461274.8754 12.07 18:12:39.23 +40:59:44.4
68.18598 24.34683 galactic Her Second-epoch detections are separated by 2.7" and 4.8 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 | 18:12:39.23 +40:59:44.4 (user input) | T | P | (position from user input) J-Ks=0.780+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:39.23 +40:59:44.4: 13.01 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:12:39.23 +40:59:44.4: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
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 08 22.3754* 18 12 39.23 +40 59 44.4 12.1 U Her 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,2461274.8754,12.07,0.05,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 20260822.3754 12.07CV 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 08 22.3754 2461274.8754 12.25 18:16:07.72 +40:27:03.1
67.81171 23.56372 galactic Lyr Second-epoch detections are separated by 1.6" 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 | ATO J274.0361+40.4578 | 18:16:07.72 +40:27:03.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.331+/-0.031 (G)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:07.72 +40:27:03.1: 13.32 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:16:07.72 +40:27:03.1: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
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
ATO J274.0361+40.4578,2461274.8754,12.25,0.05,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
ATO J274.0361+40.4578 20260822.3754 12.25CV 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 08 22.3754 2461274.8754 11.87 18:13:18.61 +35:23:19.3
62.37671 22.59530 galactic Her Second-epoch detections are separated by 4.0" and 5.0 pix
The object was found in VSX 3" GSC 02630-00495
Type: SR
# Max. Min./Amp. JD0 Period
14.120 g Y 0.450 R1 2458636.05920 82.167732100000 M6/7
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:13:18.61 +35:23:19.3: 12.93 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:13:18.61 +35:23:19.3: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
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 08 22.3754* 18 13 18.61 +35 23 19.3 11.9 U Her 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
GSC 02630-00495,2461274.8754,11.87,0.05,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
GSC 02630-00495 20260822.3754 11.87CV 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: 2461176.89547439 16.05.2026 09:29:18.987 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
First image: 2461176.89547439 16.05.2026 09:29:18.987 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Last image: 2461274.87562071 22.08.2026 09:00:43.629 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
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: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 17310
Objects passed selection criteria: 17190
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 10160.2
Average stars matched: 9472.25 (93.2285 %)
Memory usage VmPeak: 243624 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:26:41 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: 2461176.89547439 16.05.2026 09:29:18.987 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
First image: 2461176.89547439 16.05.2026 09:29:18.987 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Last image: 2461274.87562071 22.08.2026 09:00:43.629 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 106
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.09
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 25 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 117889
Objects passed selection criteria: 117462
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 74140
Average stars matched: 67616 (91.2004 %)
Memory usage VmPeak: 569500 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:28:01 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
SExtractor catalog cache: saved Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.cat to cache
SExtractor catalog cache: saved Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.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/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.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: 2461274.87515667
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_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits exists and is non-empty
wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits exists and is non-empty
wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits exists and is non-empty
wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (1st reference image)
verification OK: wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Image size: 937.5'x624.3' 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: 18:32:42.750 +37:59:52.55 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits (1st new image)
verification OK: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
Image size: 937.8'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:32:57.410 +38:00:57.58 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:32:42.750 +37:59:52.55
Second-epoch image center 18:32:57.410 +38:00:57.58
Angular distance between the image centers 0.0514 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits (2nd new image)
verification OK: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
Image size: 937.8'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:32:58.451 +38:00:35.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:32:42.750 +37:59:52.55
Second-epoch image center 18:32:58.451 +38:00:35.07
Angular distance between the image centers 0.0529 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 18:32:57.410 +38:00:57.58
Second-epoch second image center 18:32:58.451 +38:00:35.07
Angular distance between the image centers 0.00713 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits &> /tmp/tmp.pCP5SsxsXr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits &> /tmp/tmp.bNB2VmqbdZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits &> /tmp/tmp.4x2NuWrxzb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits &> /tmp/tmp.xvPgVY0XTp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.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_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
Found non-empty wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
The reference image (wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits) and catalog (wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat) found
'wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat' -> 'wcsmag.cat'
Read 25255 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.6061 to 288.8205 deg, Dec +32.4326 to +43.2588 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 267.6061 to 288.8205 deg, Dec 32.4326 to 43.2588 deg
Loaded 16483 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): 11905 out of 12949 total matches.
Matched with Tycho-2 12949 out of 25255 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.748300
a=0.000000 b=1.000000 c=22.748300
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 25255 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.6061 to 288.8205 deg, Dec +32.4326 to +43.2588 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 267.6061 to 288.8205 deg, Dec 32.4326 to 43.2588 deg
Loaded 16483 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): 11905 out of 12949 total matches.
Matched with Tycho-2 12949 out of 25255 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Forced-photometry filter: calibrated wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits -> calib.txt_param_ref_wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (aperture=6.3)
Read 25065 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.6033 to 288.8211 deg, Dec +32.4339 to +43.2688 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 267.6033 to 288.8211 deg, Dec 32.4339 to 43.2688 deg
Loaded 16494 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): 11889 out of 12942 total matches.
Matched with Tycho-2 12942 out of 25065 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Forced-photometry filter: calibrated wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
2.3 pix Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
2.1 pix fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
2.1 pix fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
Limiting magnitude estimates:
15.3 mag. Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
15.3 mag. Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
12.4 mag. fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
12.3 mag. fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
All-image limiting magnitude estimate: 12.3 (SNR ) 10.2 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.pCP5SsxsXr (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits' -> 'wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS_IMAGE_NAME=wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS-calibrated image found: wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Checking if the catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat corresponding to the image wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits alredy exist and is non-empty...
Catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat corresponding to the image wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS catalog name: wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2241, bad_region=8098, passed=25255
Got 25255 stars (including 15632 good ones) from the SExtractor catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
util/solve_plate_with_UCAC5 got 25255 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 4906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 18693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 18693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 18693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4907 stars left (next iteration limit 5396)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits N_match=4907 sigma_overall_arcsec=0.398 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.406 sigma_q4_arcsec=0.408 n_q1=1482 n_q2=1140 n_q3=1323 n_q4=962 worst_quadrant_to_overall_ratio=1.026
The image catalog is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits -region wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bNB2VmqbdZ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits' -> 'wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS-calibrated image found: wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Checking if the catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS catalog name: wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2234, bad_region=8005, passed=25065
Got 25065 stars (including 15572 good ones) from the SExtractor catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 25065 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 4906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 18615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 18615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 18615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4907 stars left (next iteration limit 5396)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits N_match=4907 sigma_overall_arcsec=0.415 sigma_q1_arcsec=0.371 sigma_q2_arcsec=0.448 sigma_q3_arcsec=0.423 sigma_q4_arcsec=0.416 n_q1=1478 n_q2=1146 n_q3=1314 n_q4=969 worst_quadrant_to_overall_ratio=1.079
The image catalog is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits -region wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4x2NuWrxzb (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_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.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_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
WCS-calibrated image found: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
Checking if the catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
WCS catalog name: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=175, bad_region=375, passed=3694
Got 3694 stars (including 3148 good ones) from the SExtractor catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat
util/solve_plate_with_UCAC5 got 3694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 3100 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3081 matched stars entering correct_measured_positions(), 3081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3081 matched stars entering correct_measured_positions(), 3416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 3100 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3081 matched stars entering correct_measured_positions(), 3416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 3081 matched stars entering correct_measured_positions(), 3416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 3081 stars left (next iteration limit 3389)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3081 robust_rms=5.097 arcsec worst_quadrant_rms=34.456 arcsec
SIP_REFIT: SIP order 3 trial: matched=3081 robust_rms=0.504 arcsec worst_quadrant_rms=0.526 arcsec
SIP_REFIT: SIP order 5 trial: matched=3081 robust_rms=0.457 arcsec worst_quadrant_rms=0.462 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3081 robust_rms_before=0.560 arcsec robust_rms_before_corrected=0.484 arcsec robust_rms_after=0.457 arcsec worst_quadrant_rms_before=0.524 worst_quadrant_rms_after=0.462
verification OK: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
verification OK: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
Image size: 938.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:32:57.409 +38:00:57.64 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3694 stars ###
'wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/correct_sextractor_wcs_catalog_usingxy2sky2260848.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.560 -> 0.457 arcsec)
WCS_QUALITY_DIAG: file=fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits N_match=3081 sigma_overall_arcsec=0.495 sigma_q1_arcsec=0.487 sigma_q2_arcsec=0.478 sigma_q3_arcsec=0.514 sigma_q4_arcsec=0.531 n_q1=1207 n_q2=331 n_q3=1253 n_q4=290 worst_quadrant_to_overall_ratio=1.073
The image catalog is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits -region wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xvPgVY0XTp (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_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.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_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
Checking if the catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
WCS catalog name: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=194, bad_region=349, passed=3716
Got 3716 stars (including 3177 good ones) from the SExtractor catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 3716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 3128 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3110 matched stars entering correct_measured_positions(), 3110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3110 matched stars entering correct_measured_positions(), 3447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 3128 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3110 matched stars entering correct_measured_positions(), 3447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 3110 matched stars entering correct_measured_positions(), 3447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 3110 stars left (next iteration limit 3421)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3110 robust_rms=5.262 arcsec worst_quadrant_rms=32.527 arcsec
SIP_REFIT: SIP order 3 trial: matched=3110 robust_rms=0.507 arcsec worst_quadrant_rms=0.552 arcsec
SIP_REFIT: SIP order 5 trial: matched=3110 robust_rms=0.454 arcsec worst_quadrant_rms=0.467 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3110 robust_rms_before=0.563 arcsec robust_rms_before_corrected=0.481 arcsec robust_rms_after=0.454 arcsec worst_quadrant_rms_before=0.498 worst_quadrant_rms_after=0.467
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.498 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits N_match=3110 sigma_overall_arcsec=0.502 sigma_q1_arcsec=0.499 sigma_q2_arcsec=0.470 sigma_q3_arcsec=0.526 sigma_q4_arcsec=0.456 n_q1=1187 n_q2=360 n_q3=1251 n_q4=312 worst_quadrant_to_overall_ratio=1.050
The image catalog is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits -region wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits to local_wcs_cache/
'wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits' -> 'local_wcs_cache/wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits'
Saving the final (post-refit) wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits to local_wcs_cache/
'wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits' -> 'local_wcs_cache/wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits'
Saving the final (post-refit) wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits to local_wcs_cache/
'wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits' -> 'local_wcs_cache/wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits'
Saving the final (post-refit) wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits to local_wcs_cache/
'wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits' -> 'local_wcs_cache/wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits sigma_overall=0.398 worst_q_ratio=1.026
ref2=Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits sigma_overall=0.415 worst_q_ratio=1.079
new1=fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits sigma_overall=0.495 worst_q_ratio=1.073
new2=fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits sigma_overall=0.502 worst_q_ratio=1.050
reference average sigma_overall=0.4065 worst_q_ratio=1.0525
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299_astrometric_residuals.png (4907 matched stars from wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300_astrometric_residuals.png (4907 matched stars from wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130_astrometric_residuals.png (3081 matched stars from wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131_astrometric_residuals.png (3110 matched stars from wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits'
Saving fully-calibrated image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits'
Preparing the HTML report for the field Lyr-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:23:56.52 +39:35:02.3: 10.76 +/- 0.00 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:23:56.52 +39:35:02.3: 10.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.00
Forced photometry filter KEPT candidate at 18:23:56.52 +39:35:02.3: ref_mag=10.76 +/- 0.00 new_mean_mag=9.6940 delta=1.07 (need > 0.90)
Adding exclusion_list_local.txt__out17233.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31075_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 31075_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:42:10.06 +34:44:49.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31084_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 31084_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:44:48.13 +37:35:42.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17233_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
Preparing report for the candidate 17233_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05599_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 05599_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:44:52.06 +34:40:34.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Lyr-02-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 ####
18:23:56.52 +39:35:02.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
SExtractor catalog cache: saved Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.cat to cache
SExtractor catalog cache: saved Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Creating symlink local_wcs_cache/wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Creating symlink local_wcs_cache/wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
Creating symlink local_wcs_cache/wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
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_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits exists and is non-empty
wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits exists and is non-empty
wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits exists and is non-empty
wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (1st reference image)
verification OK: wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Image size: 937.5'x624.3' 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: 18:32:42.750 +37:59:52.55 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits (1st new image)
verification OK: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
Image size: 938.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:32:57.409 +38:00:57.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:32:42.750 +37:59:52.55
Second-epoch image center 18:32:57.409 +38:00:57.64
Angular distance between the image centers 0.0514 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits (2nd new image)
verification OK: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
Image size: 937.8'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:32:58.451 +38:00:35.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:32:42.750 +37:59:52.55
Second-epoch image center 18:32:58.451 +38:00:35.07
Angular distance between the image centers 0.0529 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 18:32:57.409 +38:00:57.64
Second-epoch second image center 18:32:58.451 +38:00:35.07
Angular distance between the image centers 0.00714 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits &> /tmp/tmp.a7Z8Vyl9kX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits &> /tmp/tmp.DmA7TqNERV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits &> /tmp/tmp.ORKzA3pls7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits &> /tmp/tmp.OQuzpX31vZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.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_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
Found non-empty wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
The reference image (wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits) and catalog (wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat) found
'wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat' -> 'wcsmag.cat'
Read 156217 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.5359 to 288.8250 deg, Dec +32.4126 to +43.2618 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 267.5359 to 288.8250 deg, Dec 32.4126 to 43.2618 deg
Loaded 16557 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): 9794 out of 13149 total matches.
Matched with Tycho-2 13149 out of 156217 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.601950
a=0.000000 b=1.000000 c=22.601950
From vast_summary.log: estimated ref. image limiting mag.: -7.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.51
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 156217 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.5359 to 288.8250 deg, Dec +32.4126 to +43.2618 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 267.5359 to 288.8250 deg, Dec 32.4126 to 43.2618 deg
Loaded 16557 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): 9794 out of 13149 total matches.
Matched with Tycho-2 13149 out of 156217 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Forced-photometry filter: calibrated wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits -> calib.txt_param_ref_wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (aperture=4.7)
Read 156924 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.5473 to 288.8404 deg, Dec +32.4215 to +43.2719 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 267.5473 to 288.8404 deg, Dec 32.4215 to 43.2719 deg
Loaded 16566 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): 9829 out of 13152 total matches.
Matched with Tycho-2 13152 out of 156924 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Forced-photometry filter: calibrated wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 75 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
2.1 pix Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
2.0 pix fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
2.0 pix fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
Limiting magnitude estimates:
15.5 mag. Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
15.5 mag. Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
13.0 mag. fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
12.9 mag. fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.7 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.a7Z8Vyl9kX (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits' -> 'wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS_IMAGE_NAME=wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS-calibrated image found: wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Checking if the catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat corresponding to the image wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits alredy exist and is non-empty...
Catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat corresponding to the image wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS catalog name: wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=17837, bad_region=40200, passed=156159
Got 156159 stars (including 103277 good ones) from the SExtractor catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
util/solve_plate_with_UCAC5 got 156159 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4914 matched stars entering correct_measured_positions(), 4914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4914 matched stars entering correct_measured_positions(), 125521 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 125521 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 125521 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4915 stars left (next iteration limit 5405)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits N_match=4915 sigma_overall_arcsec=0.385 sigma_q1_arcsec=0.335 sigma_q2_arcsec=0.416 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.383 n_q1=1518 n_q2=1090 n_q3=1358 n_q4=949 worst_quadrant_to_overall_ratio=1.079
The image catalog is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits -region wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DmA7TqNERV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits' -> 'wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS-calibrated image found: wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Checking if the catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS catalog name: wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=17853, bad_region=40597, passed=156882
Got 156882 stars (including 103605 good ones) from the SExtractor catalog wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 156882 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 126054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 126054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 126054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4912 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits N_match=4912 sigma_overall_arcsec=0.401 sigma_q1_arcsec=0.356 sigma_q2_arcsec=0.446 sigma_q3_arcsec=0.428 sigma_q4_arcsec=0.375 n_q1=1523 n_q2=1094 n_q3=1349 n_q4=946 worst_quadrant_to_overall_ratio=1.113
The image catalog is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits -region wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ORKzA3pls7 (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_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.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_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
WCS-calibrated image found: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
Checking if the catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
WCS catalog name: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1255, bad_region=2092, passed=35326
Got 35326 stars (including 32081 good ones) from the SExtractor catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat
util/solve_plate_with_UCAC5 got 35326 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 4929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 33847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 4929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 33847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 33847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4906 stars left (next iteration limit 5396)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4906 robust_rms=4.780 arcsec worst_quadrant_rms=36.730 arcsec
SIP_REFIT: SIP order 3 trial: matched=4906 robust_rms=0.505 arcsec worst_quadrant_rms=0.531 arcsec
SIP_REFIT: SIP order 5 trial: matched=4906 robust_rms=0.454 arcsec worst_quadrant_rms=0.467 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4906 robust_rms_before=0.455 arcsec robust_rms_before_corrected=0.465 arcsec robust_rms_after=0.454 arcsec worst_quadrant_rms_before=0.473 worst_quadrant_rms_after=0.467
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.473 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits N_match=4906 sigma_overall_arcsec=0.481 sigma_q1_arcsec=0.476 sigma_q2_arcsec=0.476 sigma_q3_arcsec=0.493 sigma_q4_arcsec=0.472 n_q1=1884 n_q2=463 n_q3=2106 n_q4=453 worst_quadrant_to_overall_ratio=1.025
The image catalog is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits -region wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OQuzpX31vZ (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_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.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_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
Checking if the catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
WCS catalog name: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1256, bad_region=1975, passed=34773
Got 34773 stars (including 31635 good ones) from the SExtractor catalog wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 34773 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 4929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 4906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 33336 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.5 to 43.3)
Done reading UCAC5 zone files...
Matched 4929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 33336 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 33336 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4906 stars left (next iteration limit 5396)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4906 robust_rms=4.931 arcsec worst_quadrant_rms=34.643 arcsec
SIP_REFIT: SIP order 3 trial: matched=4906 robust_rms=0.507 arcsec worst_quadrant_rms=0.533 arcsec
SIP_REFIT: SIP order 5 trial: matched=4906 robust_rms=0.453 arcsec worst_quadrant_rms=0.462 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4906 robust_rms_before=0.569 arcsec robust_rms_before_corrected=0.481 arcsec robust_rms_after=0.453 arcsec worst_quadrant_rms_before=0.489 worst_quadrant_rms_after=0.462
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.489 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits N_match=4906 sigma_overall_arcsec=0.493 sigma_q1_arcsec=0.498 sigma_q2_arcsec=0.473 sigma_q3_arcsec=0.515 sigma_q4_arcsec=0.435 n_q1=1865 n_q2=493 n_q3=2089 n_q4=459 worst_quadrant_to_overall_ratio=1.044
The image catalog is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits -region wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.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_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-03_20.00sec_-0.00C_LIGHT_0130.fits
Saving fully-calibrated image wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.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_2026-08-22_CI_Lyr-02-Q2b1x1_042216_TTUQ2b1x1_1998867_rxBRn6Te/wcs_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131.fits
Preparing the HTML report for the field Lyr-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:49:38.06 +37:48:14.9: 11.22 +/- 0.00 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:52:52.68 +34:04:39.4: 12.62 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:49:39.40 +37:21:04.9: 11.41 +/- 0.00 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:49:32.25 +40:09:36.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:22.00 +39:57:16.0: 11.89 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:22:56.33 +37:48:55.5: 11.22 +/- 0.00 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:12:22.00 +39:57:16.0: 11.89 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:49:38.06 +37:48:14.9: 11.20 +/- 0.00 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:52:52.68 +34:04:39.4: 12.67 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:49:39.40 +37:21:04.9: 11.44 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:49:32.25 +40:09:36.6: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Forced photometry reference-image weighted average: 11.21 +/- 0.00
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter REJECTED candidate at 18:12:22.00 +39:57:16.0: ref_mag=11.89 +/- 0.01 new_mean_mag=11.3956 delta=0.49 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:49:38.06 +37:48:14.9: ref_mag=11.21 +/- 0.00 new_mean_mag=11.3224 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:52:52.68 +34:04:39.4: ref_mag=12.65 +/- 0.01 new_mean_mag=12.2747 delta=0.37 (need > 0.90)
Forced photometry reference-image weighted average: 11.43 +/- 0.00
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter REJECTED candidate at 18:49:39.40 +37:21:04.9: ref_mag=11.43 +/- 0.00 new_mean_mag=11.6191 delta=-0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:49:32.25 +40:09:36.6: ref_mag=12.70 +/- 0.01 new_mean_mag=12.5838 delta=0.12 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:22:56.33 +37:48:55.5: 11.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Forced photometry filter REJECTED candidate at 18:22:56.33 +37:48:55.5: ref_mag=11.22 +/- 0.00 new_mean_mag=11.3710 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:14:58.74 +39:44:28.3: 12.34 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:14:58.74 +39:44:28.3: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter REJECTED candidate at 18:14:58.74 +39:44:28.3: ref_mag=12.31 +/- 0.01 new_mean_mag=12.0107 delta=0.30 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:39.23 +40:59:44.4: 13.01 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:16:07.72 +40:27:03.1: 13.32 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:12:39.23 +40:59:44.4: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 18:12:39.23 +40:59:44.4: ref_mag=12.99 +/- 0.02 new_mean_mag=12.0506 delta=0.94 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:16:07.72 +40:27:03.1: 13.29 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:13:18.61 +35:23:19.3: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 18:16:07.72 +40:27:03.1: ref_mag=13.30 +/- 0.02 new_mean_mag=12.2416 delta=1.06 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q2b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:13:18.61 +35:23:19.3: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter KEPT candidate at 18:13:18.61 +35:23:19.3: ref_mag=12.97 +/- 0.02 new_mean_mag=11.8149 delta=1.15 (need > 0.90)
Adding exclusion_list_local.txt__out125146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44120.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 88s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 176655_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 176655_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (25.2") between the two second-epoch detections
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Considering the candidate 176661_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 176661_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
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Considering the candidate 176664_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 176664_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
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Considering the candidate 176665_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 176665_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
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Considering the candidate 176668_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 176668_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
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Considering the candidate 176671_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 176671_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
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Considering the candidate 176672_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 176672_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
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Considering the candidate 176683_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 176683_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:44:48.10 +37:35:42.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 179076_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 179076_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 180223_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 180223_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:49:41.59 +38:27:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180261_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 180261_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (25.2") between the two second-epoch detections
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Considering the candidate 180328_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 180328_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:54:43.86 +36:54:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180731_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 180731_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (25.9") between the two second-epoch detections
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Considering the candidate 181893_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 181893_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 182634_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 182634_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 182649_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 182649_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (27.0") between the two second-epoch detections
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Considering the candidate 183416_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 183416_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 183788_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 183788_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 183800_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 183800_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:51:36.01 +36:33:49.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 183903_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 183903_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 184060_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 184060_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:54:37.17 +36:55:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184067_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 184067_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:53:11.12 +41:01:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184209_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 184209_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:44:22.78 +39:38:18.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 184659_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 184659_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 184773_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 184773_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (25.9") between the two second-epoch detections
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Considering the candidate 184781_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 184781_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
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Considering the candidate 184860_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 184860_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
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Considering the candidate 185112_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 185112_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (24.6") between the two second-epoch detections
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Considering the candidate 185167_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 185167_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:38:16.50 +39:42:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185221_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 185221_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 185628_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 185628_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 185763_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 185763_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (25.9") between the two second-epoch detections
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Considering the candidate 185804_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 185804_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:48:36.30 +33:46:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186209_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 186209_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
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Considering the candidate 186288_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 186288_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (27.6") between the two second-epoch detections
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Considering the candidate 186385_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 186385_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 186847_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 186847_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 186937_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 186937_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (27.2") between the two second-epoch detections
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Considering the candidate 187087_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 187087_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (25.0") between the two second-epoch detections
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Considering the candidate 187436_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 187436_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 188406_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 188406_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:53:43.77 +40:18:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189095_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 189095_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
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Considering the candidate 189221_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 189221_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:35:15.19 +38:53:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189282_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 189282_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
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Considering the candidate 189341_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 189341_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 189585_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 189585_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 189763_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 189763_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 190632_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 190632_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 122472_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 122472_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:12:42.64 +41:08:47.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54863_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 54863_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:19:51.91 +36:03:55.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 136114_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 136114_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:44:22.71 +39:36:46.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74705_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 74705_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:44:46.22 +37:36:19.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31971_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 31971_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:44:52.05 +34:40:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92491_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 92491_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 125146_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
Preparing report for the candidate 125146_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
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Considering the candidate 133663_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
Preparing report for the candidate 133663_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
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Considering the candidate 126432_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 126432_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:51:26.12 +40:54:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77309_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 77309_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:30:13.26 +37:29:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78347_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 78347_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 128873_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 128873_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:43:26.02 +40:50:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113290_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 113290_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:13:39.32 +41:57:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44120_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
Preparing report for the candidate 44120_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
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Considering the candidate 58883_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 58883_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:45:31.96 +36:18:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25612_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 25612_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 145923_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 145923_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:23:56.56 +39:35:02.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 111902_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 111902_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 91647_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 91647_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 88473_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 88473_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:36:56.64 +38:47:07.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 146055_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 146055_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:38:06.37 +39:40:03.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 137121_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 137121_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:44:20.16 +39:40:13.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 147526_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 147526_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:24:13.89 +39:30:25.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 97151_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 97151_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:13:04.80 +38:46:24.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 65952_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 65952_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:54:29.76 +36:53:56.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 126515_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 126515_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks
**** FOUND 18:17:06.50 +40:56:13.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129148_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131
The candidate 129148_fd_Lyr-02-Q2b1x1_2026-08-22_04-00-43_20.00sec_-0.00C_LIGHT_0131 did not pass the final checks