This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C
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 06 22.3685 2461213.8685 11.41 22:04:21.29 -08:53:28.2
49.71055 -46.57437 galactic Aqr Second-epoch detections are separated by 0.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.354 Eleonora 0 -0 0 11.5 -0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:04:21.29 -08:53:28.2: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:04:21.29 -08:53:28.2: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461213.8685,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260622.3685 11.41CV 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 06 22.3685 2461213.8685 12.09 22:25:35.24 -10:51:06.9
51.19426 -52.07506 galactic Aqr Second-epoch detections are separated by 0.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.100 Hekate 1 -1 1 12.3 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:25:35.24 -10:51:06.9: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:25:35.24 -10:51:06.9: 15.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461213.8685,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260622.3685 12.09CV 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 06 22.3685 2461213.8685 12.89 22:30:52.58 -07:42:41.3
56.60710 -51.47962 galactic Aqr Second-epoch detections are separated by 0.2" and 3.0 pix
The object was found in VSX 1" GW Aqr
Type: RRAB
# Max. Min./Amp. JD0 Period
12.787 V 13.879 V 2453729.74600 0.525966200000
The object was not found in astcheck.
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:30:52.58 -07:42:41.3: 13.84 +/- 0.11 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:30:52.58 -07:42:41.3: 13.80 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.08
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
GW Aqr,2461213.8685,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GW Aqr 20260622.3685 12.89CV 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: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
First image: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Last image: 2461213.86875354 22.06.2026 08:50:50.306 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.05
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: 7 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): 4489
Objects passed selection criteria: 4485
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 4111.5
Average stars matched: 3829 (93.129 %)
Memory usage VmPeak: 110732 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 21 14:44:16 CDT 2026
VaST build number 1.0rc89-107-g3b0f95a5
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 22 04:21:03 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: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
First image: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Last image: 2461213.86875354 22.06.2026 08:50:50.306 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 106
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.81
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 21 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 28706
Objects passed selection criteria: 28616
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 26315
Average stars matched: 23809.2 (90.4779 %)
Memory usage VmPeak: 131240 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 21 14:44:16 CDT 2026
VaST build number 1.0rc89-107-g3b0f95a5
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 22 04:24:14 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.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: 2461213.86831248
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits exists and is non-empty
Saving wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits'
wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
Saving wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits'
wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Image size: 942.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:06.962 -09:59:19.64 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/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_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.102 -10:00:03.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:08.102 -10:00:03.28
Angular distance between the image centers 0.0130 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.292 -10:00:04.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:09.292 -10:00:04.23
Angular distance between the image centers 0.0156 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 22:17:08.102 -10:00:03.28
Second-epoch second image center 22:17:09.292 -10:00:04.23
Angular distance between the image centers 0.00489 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/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits &> /tmp/tmp.l1azWzhjcZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.0fQuQxNTGF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits &> /tmp/tmp.bqgD8z4g2i
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits &> /tmp/tmp.esNunCs6hO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Calibrating the magnitude scale
wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits does not exist or is empty: waiting for solve_plate_with_UCAC5
wait
############ /tmp/tmp.l1azWzhjcZ (1) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=254, bad_region=772, passed=4529
Got 4529 stars (including 3543 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
util/solve_plate_with_UCAC5 got 4529 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 874 matched stars entering correct_measured_positions(), 870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 874 matched stars entering correct_measured_positions(), 3782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 874 matched stars entering correct_measured_positions(), 3782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 874 matched stars entering correct_measured_positions(), 3782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 874 stars left (next iteration limit 961)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits N_match=874 sigma_overall_arcsec=0.273 sigma_q1_arcsec=0.289 sigma_q2_arcsec=0.273 sigma_q3_arcsec=0.247 sigma_q4_arcsec=0.284 n_q1=315 n_q2=125 n_q3=315 n_q4=119 worst_quadrant_to_overall_ratio=1.056
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -region wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0fQuQxNTGF (1) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=252, bad_region=782, passed=4507
Got 4507 stars (including 3517 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 4507 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 3759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 3757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 3757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 870 stars left (next iteration limit 957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits N_match=870 sigma_overall_arcsec=0.274 sigma_q1_arcsec=0.275 sigma_q2_arcsec=0.293 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.289 n_q1=313 n_q2=125 n_q3=313 n_q4=119 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bqgD8z4g2i (1) ############
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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=364, bad_region=1331, passed=5869
Got 5869 stars (including 4246 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat
util/solve_plate_with_UCAC5 got 5869 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 4679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 4680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 4680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 879 stars left (next iteration limit 966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits N_match=879 sigma_overall_arcsec=0.369 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.352 sigma_q3_arcsec=0.423 sigma_q4_arcsec=0.372 n_q1=308 n_q2=149 n_q3=288 n_q4=134 worst_quadrant_to_overall_ratio=1.144
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.esNunCs6hO (1) ############
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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=366, bad_region=1318, passed=5828
Got 5828 stars (including 4212 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat
util/solve_plate_with_UCAC5 got 5828 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 4663 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 4664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 4664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 879 stars left (next iteration limit 966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits N_match=879 sigma_overall_arcsec=0.396 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.335 sigma_q3_arcsec=0.438 sigma_q4_arcsec=0.419 n_q1=310 n_q2=149 n_q3=288 n_q4=132 worst_quadrant_to_overall_ratio=1.106
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
____ 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_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat' -> 'wcsmag.cat'
Read 4529 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 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 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 deg
Loaded 5486 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): 3405 out of 3455 total matches.
Matched with Tycho-2 3455 out of 4529 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.442200
a=0.000000 b=1.000000 c=22.442200
From vast_summary.log: estimated ref. image limiting mag.: -8.05
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.39
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 4529 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 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 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 deg
Loaded 5486 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): 3405 out of 3455 total matches.
Matched with Tycho-2 3455 out of 4529 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (aperture=6.1)
Read 4507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9176 to 342.3811 deg, Dec -15.5918 to -4.2887 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 325.9176 to 342.3811 deg, Dec -15.5918 to -4.2887 deg
Loaded 5486 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): 3392 out of 3444 total matches.
Matched with Tycho-2 3444 out of 4507 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
2.3 pix fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
2.3 pix fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
2.4 pix wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Limiting magnitude estimates:
14.4 mag. Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
14.4 mag. Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
14.6 mag. fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
14.6 mag. fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.5 (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
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits sigma_overall=0.273 worst_q_ratio=1.056
ref2=Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits sigma_overall=0.274 worst_q_ratio=1.070
new1=fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits sigma_overall=0.369 worst_q_ratio=1.144
new2=fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits sigma_overall=0.396 worst_q_ratio=1.106
reference average sigma_overall=0.2735 worst_q_ratio=1.063
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446_astrometric_residuals.png (874 matched stars from wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447_astrometric_residuals.png (870 matched stars from wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390_astrometric_residuals.png (879 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391_astrometric_residuals.png (879 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits'
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:29:00.02 -09:56:39.8: 11.61 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:21:00.92 -14:05:01.7: 11.82 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:05:36.94 -09:52:54.3: 11.47 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:23:04.68 -12:41:13.2: 11.76 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:04:21.29 -08:53:28.2: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:21:00.92 -14:05:01.7: 11.82 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:29:00.02 -09:56:39.8: 11.63 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:23:04.68 -12:41:13.2: 11.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:05:36.94 -09:52:54.3: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Forced photometry filter REJECTED candidate at 22:21:00.92 -14:05:01.7: ref_mag=11.82 +/- 0.01 new_mean_mag=11.5641 delta=0.26 (need > 0.90)
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry filter REJECTED candidate at 22:29:00.02 -09:56:39.8: ref_mag=11.62 +/- 0.01 new_mean_mag=11.3935 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:04.68 -12:41:13.2: ref_mag=11.78 +/- 0.01 new_mean_mag=11.6056 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Forced photometry filter REJECTED candidate at 22:05:36.94 -09:52:54.3: ref_mag=11.46 +/- 0.01 new_mean_mag=11.4860 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:04:21.29 -08:53:28.2: 15.04 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20239.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20235_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 20235_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20239_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
Preparing report for the candidate 20239_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20243_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 20243_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20249_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 20249_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20250_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 20250_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:04:21.29 -08:53:28.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits exists and is non-empty
wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Image size: 942.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:06.962 -09:59:19.64 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/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_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:08.102 -10:00:03.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:08.102 -10:00:03.28
Angular distance between the image centers 0.0130 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.292 -10:00:04.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:09.292 -10:00:04.23
Angular distance between the image centers 0.0156 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 22:17:08.102 -10:00:03.28
Second-epoch second image center 22:17:09.292 -10:00:04.23
Angular distance between the image centers 0.00489 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/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits &> /tmp/tmp.0apXQiC01w
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.rE8FXt4kV9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits &> /tmp/tmp.s5ijzV4RYx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits &> /tmp/tmp.cHXrhwwyX4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat' -> 'wcsmag.cat'
Read 27177 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 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 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 deg
Loaded 5550 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): 4272 out of 4485 total matches.
Matched with Tycho-2 4485 out of 27177 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.308200
a=0.000000 b=1.000000 c=22.308200
From vast_summary.log: estimated ref. image limiting mag.: -7.81
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27177 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 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 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 deg
Loaded 5550 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): 4272 out of 4485 total matches.
Matched with Tycho-2 4485 out of 27177 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (aperture=5.0)
Read 27357 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8701 to 342.4399 deg, Dec -15.6108 to -4.2411 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 325.8701 to 342.4399 deg, Dec -15.6108 to -4.2411 deg
Loaded 5555 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): 4272 out of 4487 total matches.
Matched with Tycho-2 4487 out of 27357 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
2.2 pix fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
2.1 pix fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
2.4 pix wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Limiting magnitude estimates:
14.5 mag. Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
14.5 mag. Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
14.9 mag. fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
14.9 mag. fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 13.9 (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.0apXQiC01w (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/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=866, bad_region=3938, passed=27173
Got 27173 stars (including 22429 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
util/solve_plate_with_UCAC5 got 27173 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 23413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 23413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 23413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 873 stars left (next iteration limit 960)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits N_match=873 sigma_overall_arcsec=0.282 sigma_q1_arcsec=0.287 sigma_q2_arcsec=0.296 sigma_q3_arcsec=0.270 sigma_q4_arcsec=0.322 n_q1=307 n_q2=123 n_q3=327 n_q4=116 worst_quadrant_to_overall_ratio=1.143
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -region wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rE8FXt4kV9 (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/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=827, bad_region=3918, passed=27350
Got 27350 stars (including 22680 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 27350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 23572 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 23571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 23571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 869 stars left (next iteration limit 955)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits N_match=869 sigma_overall_arcsec=0.276 sigma_q1_arcsec=0.264 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.265 sigma_q4_arcsec=0.310 n_q1=312 n_q2=122 n_q3=319 n_q4=116 worst_quadrant_to_overall_ratio=1.126
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.s5ijzV4RYx (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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1502, bad_region=5570, passed=35115
Got 35115 stars (including 28293 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat
util/solve_plate_with_UCAC5 got 35115 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 867 matched stars entering correct_measured_positions(), 862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 867 matched stars entering correct_measured_positions(), 30250 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 867 matched stars entering correct_measured_positions(), 30250 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 867 matched stars entering correct_measured_positions(), 30250 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 867 stars left (next iteration limit 953)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits N_match=867 sigma_overall_arcsec=0.364 sigma_q1_arcsec=0.302 sigma_q2_arcsec=0.376 sigma_q3_arcsec=0.397 sigma_q4_arcsec=0.340 n_q1=301 n_q2=153 n_q3=283 n_q4=130 worst_quadrant_to_overall_ratio=1.091
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cHXrhwwyX4 (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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1463, bad_region=5597, passed=35314
Got 35314 stars (including 28476 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat
util/solve_plate_with_UCAC5 got 35314 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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 868 matched stars entering correct_measured_positions(), 866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 868 matched stars entering correct_measured_positions(), 30582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 868 matched stars entering correct_measured_positions(), 30583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 868 matched stars entering correct_measured_positions(), 30583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 868 stars left (next iteration limit 954)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits N_match=868 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.386 sigma_q3_arcsec=0.421 sigma_q4_arcsec=0.403 n_q1=302 n_q2=153 n_q3=280 n_q4=133 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-12_20.00sec_4.90C_LIGHT_0390.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.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_2026-06-22_CI_Aqr-04-Q2b1x1_041823_TTUQ2b1x1_2809446_mkEBcQ8C/wcs_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391.fits
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:53:44.83 -12:38:05.7: 13.49 +/- 0.09 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:16:02.27 -06:53:46.8: 13.34 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:49:22.86 -12:25:34.2: 12.69 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:01:42.54 -09:18:55.5: 13.03 +/- 0.05 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:19:05.60 -09:54:05.0: 13.26 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:55:39.76 -08:13:10.7: 13.13 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:06:25.68 -06:07:35.4: 13.76 +/- 0.11 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:07:37.37 -13:04:59.8: 12.50 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:50:44.64 -12:34:12.0: 13.06 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:27:18.59 -09:24:59.8: 13.30 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:44.83 -12:38:05.7: 13.53 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.07
Forced photometry filter REJECTED candidate at 21:53:44.83 -12:38:05.7: ref_mag=13.51 +/- 0.07 new_mean_mag=13.8037 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:16:02.27 -06:53:46.8: 13.49 +/- 0.08 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:55:39.76 -08:13:10.7: 13.11 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:07:37.37 -13:04:59.8: 12.60 +/- 0.04 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:18.59 -09:24:59.8: 13.34 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:06:25.68 -06:07:35.4: 13.77 +/- 0.10 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:19:05.60 -09:54:05.0: 13.18 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.04
Forced photometry reference-image weighted average: 13.40 +/- 0.05
Forced photometry reference-image weighted average: 12.55 +/- 0.03
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:22.86 -12:25:34.2: 12.79 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:01:42.54 -09:18:55.5: 13.05 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:50:44.64 -12:34:12.0: 13.29 +/- 0.09 detection
Forced photometry filter REJECTED candidate at 22:16:02.27 -06:53:46.8: ref_mag=13.40 +/- 0.05 new_mean_mag=13.7269 delta=-0.33 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:07:37.37 -13:04:59.8: ref_mag=12.55 +/- 0.03 new_mean_mag=12.9032 delta=-0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:55:39.76 -08:13:10.7: ref_mag=13.12 +/- 0.04 new_mean_mag=13.6721 delta=-0.55 (need > 0.90)
Forced photometry reference-image weighted average: 13.77 +/- 0.08
Forced photometry reference-image weighted average: 12.73 +/- 0.04
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Forced photometry reference-image weighted average: 13.15 +/- 0.05
Forced photometry reference-image weighted average: 13.04 +/- 0.04
Forced photometry reference-image weighted average: 13.32 +/- 0.05
Forced photometry filter REJECTED candidate at 22:19:05.60 -09:54:05.0: ref_mag=13.22 +/- 0.04 new_mean_mag=13.6130 delta=-0.40 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:06:25.68 -06:07:35.4: ref_mag=13.77 +/- 0.08 new_mean_mag=13.9023 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:49:22.86 -12:25:34.2: ref_mag=12.73 +/- 0.04 new_mean_mag=13.1199 delta=-0.39 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:50:44.64 -12:34:12.0: ref_mag=13.15 +/- 0.05 new_mean_mag=13.4556 delta=-0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:01:42.54 -09:18:55.5: ref_mag=13.04 +/- 0.04 new_mean_mag=13.4668 delta=-0.42 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:27:18.59 -09:24:59.8: ref_mag=13.32 +/- 0.05 new_mean_mag=13.5479 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:12:19.39 -10:03:21.6: 12.49 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:07:46.40 -05:55:05.6: 11.48 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:56:23.34 -11:50:35.6: 12.23 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:25:35.24 -10:51:06.9: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:52:31.30 -13:22:07.4: 12.82 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:12:19.39 -10:03:21.6: 12.45 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:27:20.27 -06:01:00.6: 12.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Forced photometry filter REJECTED candidate at 22:12:19.39 -10:03:21.6: ref_mag=12.47 +/- 0.02 new_mean_mag=12.7854 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:23.34 -11:50:35.6: 12.25 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:07:46.40 -05:55:05.6: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Forced photometry filter REJECTED candidate at 21:56:23.34 -11:50:35.6: ref_mag=12.24 +/- 0.02 new_mean_mag=12.5922 delta=-0.35 (need > 0.90)
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Forced photometry filter REJECTED candidate at 22:07:46.40 -05:55:05.6: ref_mag=11.46 +/- 0.01 new_mean_mag=11.8892 delta=-0.43 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:25:35.24 -10:51:06.9: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:21:00.19 -11:44:26.4: 13.17 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:52:31.30 -13:22:07.4: 12.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.04
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:20.27 -06:01:00.6: 13.02 +/- 0.06 detection
Forced photometry filter REJECTED candidate at 21:52:31.30 -13:22:07.4: ref_mag=12.86 +/- 0.04 new_mean_mag=12.9063 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.95 +/- 0.04
Forced photometry filter REJECTED candidate at 22:27:20.27 -06:01:00.6: ref_mag=12.95 +/- 0.04 new_mean_mag=13.0250 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:33:03.21 -11:16:50.3: 14.33 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:27:56.06 -13:47:51.8: 13.74 +/- 0.11 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:34:00.05 -12:09:43.9: 14.01 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:21:00.19 -11:44:26.4: 13.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.04
Forced photometry filter REJECTED candidate at 22:21:00.19 -11:44:26.4: ref_mag=13.14 +/- 0.04 new_mean_mag=13.4769 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:31:31.41 -06:59:54.9: 13.84 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:33:03.21 -11:16:50.3: 14.56 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:09:15.48 -13:50:29.0: 14.15 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:56.06 -13:47:51.8: 13.53 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.14
Forced photometry filter REJECTED candidate at 22:33:03.21 -11:16:50.3: ref_mag=14.42 +/- 0.14 new_mean_mag=13.9179 delta=0.50 (need > 0.90)
Forced photometry reference-image weighted average: 13.61 +/- 0.07
Forced photometry filter REJECTED candidate at 22:27:56.06 -13:47:51.8: ref_mag=13.61 +/- 0.07 new_mean_mag=13.8445 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:34:00.05 -12:09:43.9: 13.97 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.10
Forced photometry filter REJECTED candidate at 22:34:00.05 -12:09:43.9: ref_mag=13.99 +/- 0.10 new_mean_mag=13.9304 delta=0.06 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:10:58.34 -13:38:36.5: 14.32 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:31:31.41 -06:59:54.9: 13.85 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.08
Forced photometry filter REJECTED candidate at 22:31:31.41 -06:59:54.9: ref_mag=13.85 +/- 0.08 new_mean_mag=14.0028 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:09:15.48 -13:50:29.0: 14.16 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.12
Forced photometry filter REJECTED candidate at 22:09:15.48 -13:50:29.0: ref_mag=14.15 +/- 0.12 new_mean_mag=13.9913 delta=0.16 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:57:58.35 -14:05:45.1: 13.71 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:08:10.19 -06:22:05.7: 13.97 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:10:58.34 -13:38:36.5: 14.16 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.12
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:58:10.01 -12:45:33.7: 13.96 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 22:10:58.34 -13:38:36.5: ref_mag=14.23 +/- 0.12 new_mean_mag=13.9940 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:56:46.31 -13:00:42.6: 13.90 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:49:31.89 -14:03:41.9: 14.11 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:59:40.24 -10:41:06.1: 14.04 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:08:10.19 -06:22:05.7: 13.87 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:57:58.35 -14:05:45.1: 13.92 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.09
Forced photometry reference-image weighted average: 13.92 +/- 0.09
Forced photometry filter REJECTED candidate at 21:57:58.35 -14:05:45.1: ref_mag=13.80 +/- 0.09 new_mean_mag=13.9695 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:08:10.19 -06:22:05.7: ref_mag=13.92 +/- 0.09 new_mean_mag=13.8795 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:54:14.48 -11:51:54.2: 14.00 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:46.31 -13:00:42.6: 14.15 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:58:10.01 -12:45:33.7: 14.03 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.11
Forced photometry reference-image weighted average: 13.99 +/- 0.10
Forced photometry filter REJECTED candidate at 21:56:46.31 -13:00:42.6: ref_mag=13.99 +/- 0.11 new_mean_mag=13.9655 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:58:10.01 -12:45:33.7: ref_mag=13.99 +/- 0.10 new_mean_mag=14.0499 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:51:46.18 -13:12:34.2: 13.91 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:31.89 -14:03:41.9: 13.67 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.11
Forced photometry filter REJECTED candidate at 21:49:31.89 -14:03:41.9: ref_mag=13.80 +/- 0.11 new_mean_mag=13.9989 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:59:40.24 -10:41:06.1: 14.08 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.10
Forced photometry filter REJECTED candidate at 21:59:40.24 -10:41:06.1: ref_mag=14.06 +/- 0.10 new_mean_mag=13.9224 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:53:10.17 -13:18:25.7: 13.97 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:54:14.48 -11:51:54.2: 14.12 +/- 0.18 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:51:46.18 -13:12:34.2: 13.86 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.12
Forced photometry filter REJECTED candidate at 21:54:14.48 -11:51:54.2: ref_mag=14.05 +/- 0.12 new_mean_mag=14.0223 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.88 +/- 0.10
Forced photometry filter REJECTED candidate at 21:51:46.18 -13:12:34.2: ref_mag=13.88 +/- 0.10 new_mean_mag=13.9688 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:49:42.78 -12:29:01.1: 14.38 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:52:20.63 -11:04:33.7: 14.31 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:10.17 -13:18:25.7: 14.22 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.13
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:56:20.54 -08:00:34.1: 14.15 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 21:53:10.17 -13:18:25.7: ref_mag=14.07 +/- 0.13 new_mean_mag=13.9747 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:49:54.54 -07:44:53.1: 14.48 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:51:27.87 -08:34:11.3: 14.08 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:42.78 -12:29:01.1: 14.14 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.15
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:52:20.63 -11:04:33.7: 14.18 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 21:49:42.78 -12:29:01.1: ref_mag=14.23 +/- 0.15 new_mean_mag=13.9084 delta=0.32 (need > 0.90)
Forced photometry reference-image weighted average: 14.24 +/- 0.14
Forced photometry filter REJECTED candidate at 21:52:20.63 -11:04:33.7: ref_mag=14.24 +/- 0.14 new_mean_mag=14.0741 delta=0.17 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:30:52.58 -07:42:41.3: 13.84 +/- 0.11 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:20.54 -08:00:34.1: 14.03 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.10
Forced photometry filter REJECTED candidate at 21:56:20.54 -08:00:34.1: ref_mag=14.08 +/- 0.10 new_mean_mag=14.0286 delta=0.05 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:54.54 -07:44:53.1: 14.57 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.17
Forced photometry filter REJECTED candidate at 21:49:54.54 -07:44:53.1: ref_mag=14.52 +/- 0.17 new_mean_mag=13.9905 delta=0.53 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:51:27.87 -08:34:11.3: 14.08 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.11
Forced photometry filter REJECTED candidate at 21:51:27.87 -08:34:11.3: ref_mag=14.08 +/- 0.11 new_mean_mag=14.0682 delta=0.01 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:30:52.58 -07:42:41.3: 13.80 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.08
Forced photometry filter KEPT candidate at 22:30:52.58 -07:42:41.3: ref_mag=13.82 +/- 0.08 new_mean_mag=12.8906 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out19331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32085.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31949_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31949_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31956_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31956_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31957_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31957_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31958_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31958_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31962_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31962_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31963_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31963_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31965_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31965_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31966_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31966_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31967_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31967_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31969_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31969_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31970_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31970_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31971_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31971_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31975_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31975_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31995_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 31995_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32008_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32008_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32013_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32013_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32032_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32032_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32050_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32050_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
**** FOUND 22:04:21.28 -08:53:28.2 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32085_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
Preparing report for the candidate 32085_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32114_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32114_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32162_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32162_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32172_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32172_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32239_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32239_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32244_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32244_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32263_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32263_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32291_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32291_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32335_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32335_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32340_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32340_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32360_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32360_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32368_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32368_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32402_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32402_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32406_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32406_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32422_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32422_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32469_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32469_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32470_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32470_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32473_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32473_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32485_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32485_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32486_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32486_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32490_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32490_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32507_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32507_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32550_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32550_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32584_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32584_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32629_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32629_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32640_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32640_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32649_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32649_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32673_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32673_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32675_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32675_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32683_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32683_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32705_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32705_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32827_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32827_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32840_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32840_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32868_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32868_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32964_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 32964_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33036_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391
The candidate 33036_fd_Aqr-04-Q2b1x1_2026-06-22_03-50-50_20.00sec_4.90C_LIGHT_0391 did not pass the final checks