This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 28.1226 2461188.6226 10.06 08:33:54.97 -06:05:30.6
230.88439 19.52767 galactic Hya Second-epoch detections are separated by 0.4" and 8.7 pix
The object was found in VSX 0" ASAS J083355-0605.5
Type: MISC
# Max. Min./Amp. JD0 Period
10.460 V Y 0.470 V 2452686.50000 187.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:33:54.97 -06:05:30.6: 11.19 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:33:54.97 -06:05:30.6: 11.00 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.08 +/- 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
ASAS J083355-0605.5,2461188.6226,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J083355-0605.5 20260528.1226 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.1226 2461188.6226 10.03 08:18:50.03 -03:06:39.5
226.15361 17.81742 galactic Hya Second-epoch detections are separated by 0.2" and 8.6 pix
The object was found in VSX 1" ASAS J081850-0306.7
Type: SRB
# Max. Min./Amp. JD0 Period
11.100 V 12.700 V 2452750.00000 105.900000000000
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:50.03 -03:06:39.5: 11.06 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:18:50.03 -03:06:39.5: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.01 +/- 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
ASAS J081850-0306.7,2461188.6226,10.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J081850-0306.7 20260528.1226 10.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.1226 2461188.6226 10.99 08:10:28.49 -02:14:15.4
224.28308 16.43002 galactic Mon Second-epoch detections are separated by 0.6" and 8.8 pix
The object was found in VSX 2" ASAS J081028-0214.2
Type: MISC
# Max. Min./Amp. JD0 Period
12.690 V Y 1.090 V 2452187.30000 126.600000000000 M7/8
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:10:28.49 -02:14:15.4: 12.12 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:10:28.49 -02:14:15.4: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
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
ASAS J081028-0214.2,2461188.6226,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J081028-0214.2 20260528.1226 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.1226 2461188.6226 12.73 08:42:02.27 -05:29:37.3
231.47966 21.55933 galactic Hya Second-epoch detections are separated by 1.9" and 8.7 pix
The object was found in VSX 1" NSVS J0842023-052936
Type: L:
# Max. Min./Amp. JD0 Period
12.215 R1 Y 0.564 R1 110.000000000000 M4/5
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:42:02.27 -05:29:37.3: 13.70 +/- 0.05 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:42:02.27 -05:29:37.3: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
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
NSVS J0842023-052936,2461188.6226,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0842023-052936 20260528.1226 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.1226 2461188.6226 11.56 08:22:37.28 -03:52:15.4
227.34293 18.25550 galactic Hya Second-epoch detections are separated by 1.2" and 8.7 pix
The object was found in VSX 1" ASAS J082237-0352.3
Type: MISC
# Max. Min./Amp. JD0 Period
13.200 V Y 0.500 V 2452090.40000 148.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:37.28 -03:52:15.4: 12.78 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:22:37.28 -03:52:15.4: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
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
ASAS J082237-0352.3,2461188.6226,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J082237-0352.3 20260528.1226 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.1226 2461188.6226 11.87 08:33:11.62 -01:30:08.6
226.57629 21.72837 galactic Hya Second-epoch detections are separated by 2.0" and 8.9 pix
The object was found in VSX 0" NSVS J0833117-013010
Type: L:
# Max. Min./Amp. JD0 Period
11.011 R1 Y 0.478 R1 61.000000000000 M5/6
The object was not found in astcheck.
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:33:11.62 -01:30:08.6: 13.28 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:33:11.62 -01:30:08.6: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
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
NSVS J0833117-013010,2461188.6226,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0833117-013010 20260528.1226 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: 2461082.73532609 11.02.2026 05:38:42.174 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
First image: 2461082.73532609 11.02.2026 05:38:42.174 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Last image: 2461188.62288150 28.05.2026 02:56:46.962 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.78
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: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 14825
Objects passed selection criteria: 14764
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 10336
Average stars matched: 9692.75 (93.7766 %)
Memory usage VmPeak: 120144 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed May 27 21:59:41 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: 2461082.73532609 11.02.2026 05:38:42.174 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
First image: 2461082.73532609 11.02.2026 05:38:42.174 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Last image: 2461188.62288150 28.05.2026 02:56:46.962 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 26
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.44
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: 14 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 88415
Objects passed selection criteria: 88237
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 60714.8
Average stars matched: 59073.8 (97.2972 %)
Memory usage VmPeak: 2121488 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed May 27 22:02:19 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
SExtractor catalog cache: saved Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat to cache
SExtractor catalog cache: saved Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.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/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.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: 2461188.62232789
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits exists and is non-empty
Saving wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits to local_wcs_cache/
'wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits' -> 'local_wcs_cache/wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits'
wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits exists and is non-empty
Saving wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits to local_wcs_cache/
'wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits' -> 'local_wcs_cache/wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits'
wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits exists and is non-empty
Saving wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits to local_wcs_cache/
'wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits' -> 'local_wcs_cache/wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits'
wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits exists and is non-empty
Saving wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits to local_wcs_cache/
'wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits' -> 'local_wcs_cache/wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits (1st reference image)
verification OK: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:17.999 -01:59:50.01 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits (1st new image)
verification OK: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
Image size: 941.4'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:22.192 -01:59:50.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:17.999 -01:59:50.01
Second-epoch image center 08:34:22.192 -01:59:50.33
Angular distance between the image centers 0.0175 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits (2nd new image)
verification OK: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
Image size: 941.4'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:19.355 -01:59:21.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:34:17.999 -01:59:50.01
Second-epoch image center 08:34:19.355 -01:59:21.62
Angular distance between the image centers 0.0097 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 08:34:22.192 -01:59:50.33
Second-epoch second image center 08:34:19.355 -01:59:21.62
Angular distance between the image centers 0.01425 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits &> /tmp/tmp.RArNfI6xGs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits &> /tmp/tmp.4swNuQSNxM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits &> /tmp/tmp.nlXxejgNFV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits &> /tmp/tmp.b6qAprkATT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.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_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
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_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
Found non-empty wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
The reference image (wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits) and catalog (wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat) found
'wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat' -> 'wcsmag.cat'
Read 15397 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6688 to 136.5116 deg, Dec -7.3043 to +3.3173 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 120.6688 to 136.5116 deg, Dec -7.3043 to 3.3173 deg
Loaded 10194 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): 8099 out of 8827 total matches.
Matched with Tycho-2 8827 out of 15397 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.877700
a=0.000000 b=1.000000 c=22.877700
From vast_summary.log: estimated ref. image limiting mag.: -7.78
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.10
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.10
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 15397 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6688 to 136.5116 deg, Dec -7.3043 to +3.3173 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 120.6688 to 136.5116 deg, Dec -7.3043 to 3.3173 deg
Loaded 10194 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): 8099 out of 8827 total matches.
Matched with Tycho-2 8827 out of 15397 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits:
Forced-photometry filter: calibrated wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits -> calib.txt_param_ref_wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits (aperture=6.4)
Read 17191 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6917 to 136.5012 deg, Dec -7.2983 to +3.3042 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 120.6917 to 136.5012 deg, Dec -7.2983 to 3.3042 deg
Loaded 10153 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): 8425 out of 8877 total matches.
Matched with Tycho-2 8877 out of 17191 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits:
Forced-photometry filter: calibrated wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits -> calib.txt_param_ref_wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
2.5 pix Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
4.4 pix fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
4.4 pix fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
2.2 pix wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
2.5 pix wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Limiting magnitude estimates:
15.1 mag. Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
15.1 mag. Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
13.1 mag. fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
13.1 mag. fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.RArNfI6xGs (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_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits' -> 'wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS-calibrated image found: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Checking if the catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS catalog name: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1476, passed=15397
Got 15397 stars (including 13898 good ones) from the SExtractor catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
util/solve_plate_with_UCAC5 got 15397 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 14967 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
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 14964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 14965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits N_match=930 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.479 sigma_q2_arcsec=0.417 sigma_q3_arcsec=0.450 sigma_q4_arcsec=0.426 n_q1=263 n_q2=220 n_q3=237 n_q4=210 worst_quadrant_to_overall_ratio=1.042
The image catalog is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits -region wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4swNuQSNxM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits' -> 'wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS-calibrated image found: wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Checking if the catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS catalog name: wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1131, passed=17191
Got 17191 stars (including 16043 good ones) from the SExtractor catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat
util/solve_plate_with_UCAC5 got 17191 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 16766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 16766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 16766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits N_match=930 sigma_overall_arcsec=0.455 sigma_q1_arcsec=0.376 sigma_q2_arcsec=0.579 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.459 n_q1=179 n_q2=260 n_q3=197 n_q4=294 worst_quadrant_to_overall_ratio=1.274
The image catalog is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits -region wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nlXxejgNFV (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=228, passed=4479
Got 4479 stars (including 4251 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 4479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 4424 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 4422 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 4422 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 918 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits N_match=918 sigma_overall_arcsec=0.544 sigma_q1_arcsec=0.565 sigma_q2_arcsec=0.736 sigma_q3_arcsec=0.440 sigma_q4_arcsec=0.555 n_q1=192 n_q2=243 n_q3=234 n_q4=249 worst_quadrant_to_overall_ratio=1.354
The image catalog is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits -region wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.b6qAprkATT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
Checking if the catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
WCS catalog name: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=230, passed=4556
Got 4556 stars (including 4325 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat
util/solve_plate_with_UCAC5 got 4556 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 4476 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 4476 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 4477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 917 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits N_match=917 sigma_overall_arcsec=0.549 sigma_q1_arcsec=0.513 sigma_q2_arcsec=0.722 sigma_q3_arcsec=0.446 sigma_q4_arcsec=0.557 n_q1=192 n_q2=241 n_q3=231 n_q4=253 worst_quadrant_to_overall_ratio=1.316
The image catalog is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits -region wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits sigma_overall=0.459 worst_q_ratio=1.042
ref2=Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits sigma_overall=0.455 worst_q_ratio=1.274
new1=fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits sigma_overall=0.544 worst_q_ratio=1.354
new2=fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits sigma_overall=0.549 worst_q_ratio=1.316
reference average sigma_overall=0.457 worst_q_ratio=1.158
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207_astrometric_residuals.png (930 matched stars from wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085_astrometric_residuals.png (930 matched stars from wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020_astrometric_residuals.png (918 matched stars from wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021_astrometric_residuals.png (917 matched stars from wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits'
Saving fully-calibrated image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits'
Preparing the HTML report for the field Hya-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:50.03 -03:06:39.5: 11.06 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:33:54.97 -06:05:30.6: 11.19 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:33:54.97 -06:05:30.6: 11.00 +/- 0.00 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:18:50.03 -03:06:39.5: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.00
Forced photometry reference-image weighted average: 11.01 +/- 0.00
Forced photometry filter KEPT candidate at 08:33:54.97 -06:05:30.6: ref_mag=11.08 +/- 0.00 new_mean_mag=10.0574 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 08:18:50.03 -03:06:39.5: ref_mag=11.01 +/- 0.00 new_mean_mag=10.0262 delta=0.98 (need > 0.90)
Adding exclusion_list_local.txt__out01918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06612.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 01918_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
Preparing report for the candidate 01918_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06612_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
Preparing report for the candidate 06612_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01433_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 01433_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:29:41.19 -06:19:05.9 in the exclusion list exclusion_list_tycho2.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Hya-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:33:54.97 -06:05:30.6
08:18:50.03 -03:06:39.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
SExtractor catalog cache: saved Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat to cache
SExtractor catalog cache: saved Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Creating symlink local_wcs_cache/wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits exists and is non-empty
wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits exists and is non-empty
wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits exists and is non-empty
wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits (1st reference image)
verification OK: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:17.999 -01:59:50.01 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits (1st new image)
verification OK: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
Image size: 941.4'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:22.192 -01:59:50.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:17.999 -01:59:50.01
Second-epoch image center 08:34:22.192 -01:59:50.33
Angular distance between the image centers 0.0175 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits (2nd new image)
verification OK: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
Image size: 941.4'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:19.355 -01:59:21.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:34:17.999 -01:59:50.01
Second-epoch image center 08:34:19.355 -01:59:21.62
Angular distance between the image centers 0.0097 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 08:34:22.192 -01:59:50.33
Second-epoch second image center 08:34:19.355 -01:59:21.62
Angular distance between the image centers 0.01425 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits &> /tmp/tmp.5w0glSdCnU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits &> /tmp/tmp.ASyODep7Zf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits &> /tmp/tmp.pFBkuKyg1q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits &> /tmp/tmp.LMFee3ywoJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.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_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
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_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
Found non-empty wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
The reference image (wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits) and catalog (wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat) found
'wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat' -> 'wcsmag.cat'
Read 104097 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6664 to 136.5280 deg, Dec -7.3049 to +3.3189 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 120.6664 to 136.5280 deg, Dec -7.3049 to 3.3189 deg
Loaded 10204 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): 7147 out of 9101 total matches.
Matched with Tycho-2 9101 out of 104097 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.721500
a=0.000000 b=1.000000 c=22.721500
From vast_summary.log: estimated ref. image limiting mag.: -7.44
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 104097 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6664 to 136.5280 deg, Dec -7.3049 to +3.3189 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 120.6664 to 136.5280 deg, Dec -7.3049 to 3.3189 deg
Loaded 10204 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): 7147 out of 9101 total matches.
Matched with Tycho-2 9101 out of 104097 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits:
Forced-photometry filter: calibrated wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits -> calib.txt_param_ref_wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits (aperture=4.7)
Read 94372 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6830 to 136.5033 deg, Dec -7.2984 to +3.3115 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 120.6830 to 136.5033 deg, Dec -7.2984 to 3.3115 deg
Loaded 10170 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): 7417 out of 8998 total matches.
Matched with Tycho-2 8998 out of 94372 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits:
Forced-photometry filter: calibrated wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits -> calib.txt_param_ref_wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits (aperture=5.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
2.4 pix Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
3.8 pix fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
3.8 pix fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
2.0 pix wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
2.4 pix wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Limiting magnitude estimates:
15.3 mag. Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
15.2 mag. Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
13.2 mag. fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
13.2 mag. fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5w0glSdCnU (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_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits' -> 'wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS-calibrated image found: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
Checking if the catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits
WCS catalog name: wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=9087, passed=104070
Got 104070 stars (including 94791 good ones) from the SExtractor catalog wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat
util/solve_plate_with_UCAC5 got 104070 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 102214 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
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 102208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 102209 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits N_match=931 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.488 sigma_q2_arcsec=0.434 sigma_q3_arcsec=0.455 sigma_q4_arcsec=0.446 n_q1=264 n_q2=221 n_q3=243 n_q4=203 worst_quadrant_to_overall_ratio=1.063
The image catalog is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits -region wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ASyODep7Zf (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits' -> 'wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS-calibrated image found: wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
Checking if the catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat corresponding to the image wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits
WCS catalog name: wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=8013, passed=94354
Got 94354 stars (including 86210 good ones) from the SExtractor catalog wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat
util/solve_plate_with_UCAC5 got 94354 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 91878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 91878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 91876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits N_match=929 sigma_overall_arcsec=0.450 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.562 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.488 n_q1=180 n_q2=271 n_q3=179 n_q4=299 worst_quadrant_to_overall_ratio=1.247
The image catalog is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits -region wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.pFBkuKyg1q (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=2, blended=750, passed=22955
Got 22955 stars (including 22185 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 22955 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 22655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 22656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 22656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits N_match=914 sigma_overall_arcsec=0.545 sigma_q1_arcsec=0.596 sigma_q2_arcsec=0.640 sigma_q3_arcsec=0.409 sigma_q4_arcsec=0.540 n_q1=200 n_q2=242 n_q3=234 n_q4=238 worst_quadrant_to_overall_ratio=1.174
The image catalog is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits -region wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LMFee3ywoJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
Checking if the catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
WCS catalog name: wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=783, passed=23350
Got 23350 stars (including 22548 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat
util/solve_plate_with_UCAC5 got 23350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 22996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 22996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 22996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits N_match=914 sigma_overall_arcsec=0.536 sigma_q1_arcsec=0.526 sigma_q2_arcsec=0.690 sigma_q3_arcsec=0.443 sigma_q4_arcsec=0.498 n_q1=198 n_q2=242 n_q3=231 n_q4=243 worst_quadrant_to_overall_ratio=1.287
The image catalog is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits -region wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits.cat.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_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-55-59_20.00sec_-0.00C_LIGHTs_0020.fits
Saving fully-calibrated image wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Hya-03-Q1b1x1_215721_TTUQ1b1x1_3391003_F36s6VWr/wcs_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021.fits
Preparing the HTML report for the field Hya-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:46:41.37 -00:20:37.6: 12.67 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:09:25.67 -05:18:08.3: 12.26 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:04:17.08 -01:54:44.8: 11.97 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:41:18.06 -06:32:35.4: 12.11 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:46:41.37 -00:20:37.6: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter REJECTED candidate at 08:46:41.37 -00:20:37.6: ref_mag=12.63 +/- 0.01 new_mean_mag=12.4348 delta=0.20 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:09:25.67 -05:18:08.3: 12.21 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:04:17.08 -01:54:44.8: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry filter REJECTED candidate at 08:09:25.67 -05:18:08.3: ref_mag=12.24 +/- 0.01 new_mean_mag=12.5431 delta=-0.31 (need > 0.90)
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Forced photometry filter REJECTED candidate at 08:04:17.08 -01:54:44.8: ref_mag=11.98 +/- 0.01 new_mean_mag=12.2378 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:41:18.06 -06:32:35.4: 11.91 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:05.55 -02:03:10.9: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter REJECTED candidate at 08:41:18.06 -06:32:35.4: ref_mag=12.00 +/- 0.01 new_mean_mag=12.1620 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:10:28.49 -02:14:15.4: 12.12 +/- 0.01 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:42:02.27 -05:29:37.3: 13.70 +/- 0.05 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:17:05.55 -02:03:10.9: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter REJECTED candidate at 08:17:05.55 -02:03:10.9: ref_mag=12.36 +/- 0.01 new_mean_mag=12.1834 delta=0.18 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:10:28.49 -02:14:15.4: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 08:10:28.49 -02:14:15.4: ref_mag=12.00 +/- 0.01 new_mean_mag=10.9926 delta=1.01 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:42:02.27 -05:29:37.3: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 08:42:02.27 -05:29:37.3: ref_mag=13.74 +/- 0.04 new_mean_mag=12.7256 delta=1.01 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:37.28 -03:52:15.4: 12.78 +/- 0.02 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:26:06.15 -04:54:02.9: 9.17 +/- 0.00 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-02-10_23-38-42_20.00sec_-15.00C_LIGHT_0207.fits at 08:33:11.62 -01:30:08.6: 13.28 +/- 0.03 detection
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:22:37.28 -03:52:15.4: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 08:22:37.28 -03:52:15.4: ref_mag=12.52 +/- 0.01 new_mean_mag=11.5573 delta=0.96 (need > 0.90)
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:26:06.15 -04:54:02.9: 8.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 8.98 +/- 0.00
Forced photometry on wcs_Hya-03-Q1b1x1_2026-03-22_00-22-31_20.00sec_-15.00C_LIGHT_0085.fits at 08:33:11.62 -01:30:08.6: 12.66 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 08:26:06.15 -04:54:02.9: ref_mag=8.98 +/- 0.00 new_mean_mag=8.1026 delta=0.88 (need > 0.90)
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 08:33:11.62 -01:30:08.6: ref_mag=12.81 +/- 0.01 new_mean_mag=11.8615 delta=0.95 (need > 0.90)
Adding exclusion_list_local.txt__out17979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59716.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
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Considering the candidate 120003_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120003_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
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Considering the candidate 120007_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120007_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
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Considering the candidate 120230_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120230_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:08:36.91 -02:57:03.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 120345_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120345_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:24:35.68 -04:44:44.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 120347_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120347_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
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Considering the candidate 120377_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120377_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:24:35.00 -04:41:24.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 120382_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120382_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 09:05:13.52 +02:23:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120413_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120413_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
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Considering the candidate 120453_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120453_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:22:32.79 -06:12:04.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 120455_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120455_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:35:46.21 -00:25:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120474_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 120474_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:46:15.96 +01:35:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54731_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 54731_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
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Considering the candidate 114472_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 114472_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:30:44.57 -06:15:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52367_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
Preparing report for the candidate 52367_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
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Considering the candidate 17979_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
Preparing report for the candidate 17979_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
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Considering the candidate 11566_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 11566_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:33:54.96 -06:05:30.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 12938_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 12938_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:39:38.75 -05:58:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35012_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
Preparing report for the candidate 35012_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
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Considering the candidate 06206_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 06206_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:16:50.57 -06:39:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23122_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 23122_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
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Considering the candidate 42670_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 42670_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:18:50.02 -03:06:39.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 21874_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 21874_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:03:36.16 -05:09:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59716_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
Preparing report for the candidate 59716_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
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Considering the candidate 08233_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 08233_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:29:41.21 -06:19:06.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 32784_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 32784_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 08:25:39.69 -03:54:17.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 43345_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021
The candidate 43345_fd_Hya-03-Q1b1x1_2026-05-27_21-56-46_20.00sec_-0.00C_LIGHTs_0021 did not pass the final checks
