This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9
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 10.4451 2461201.9451 13.57 18:51:14.89 -04:43:04.6
28.70952 -2.10727 galactic Sct Second-epoch detections are separated by 0.8" and 11.9 pix
The object was found in VSX21" ZTF J185116.27-044304.8
Type: EW
# Max. Min./Amp. JD0 Period
19.153 r Y 0.469 r 2458425.58350 0.633685200000
The object was found in astcheck.663 Gerlinde -1 -0 1 13.8 0 0
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:51:14.89 -04:43:04.6: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:51:14.89 -04:43:04.6: 15.49 +/- 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
ZTF J185116.27-044304.8,2461201.9451,13.57,0.05,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
ZTF J185116.27-044304.8 20260610.4451 13.57CV 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 10.4451 2461201.9451 12.23 18:42:08.51 -02:45:11.3
29.42185 0.81052 galactic Aql Second-epoch detections are separated by 2.1" and 11.6 pix
The object was found in VSX 4" NSV 11221
Type: SR
# Max. Min./Amp. JD0 Period
13.300 V 15.500 V 2458215.89050 193.215772200000 M6
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:42:08.51 -02:45:11.3: 13.26 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:42:08.51 -02:45:11.3: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
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
NSV 11221,2461201.9451,12.23,0.05,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
NSV 11221 20260610.4451 12.23CV 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 10.4451 2461201.9451 12.72 18:34:24.86 +01:27:27.5
32.28890 4.45206 galactic Ser Second-epoch detections are separated by 1.0" and 11.5 pix
The object was found in VSX 6" NSVS J1834250+012735
Type: SR
# Max. Min./Amp. JD0 Period
13.143 r Y 0.870 r 2458342.66230 185.885766100000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:34:24.86 +01:27:27.5: 13.78 +/- 0.07 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:34:24.86 +01:27:27.5: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 10.4451* 18 34 24.86 +01 27 27.5 12.7 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1834250+012735,2461201.9451,12.72,0.05,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
NSVS J1834250+012735 20260610.4451 12.72CV 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: 2461175.86503943 15.05.2026 08:45:29.407 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
First image: 2461175.86503943 15.05.2026 08:45:29.407 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
Last image: 2461201.94542294 10.06.2026 10:41:14.542 /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.97
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 10551
Objects passed selection criteria: 10511
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 7439
Average stars matched: 6855.5 (92.1562 %)
Memory usage VmPeak: 116216 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jun 10 06:02:48 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: 2461175.86503943 15.05.2026 08:45:29.407 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
First image: 2461175.86503943 15.05.2026 08:45:29.407 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
Last image: 2461201.94542294 10.06.2026 10:41:14.542 /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 89
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
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: 63 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): 115866
Objects passed selection criteria: 115606
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 85677.5
Average stars matched: 76559.2 (89.3575 %)
Memory usage VmPeak: 2009144 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jun 10 06:07:48 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/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.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/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.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: 2461201.94469426
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_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits'
wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits'
wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits'
wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits (1st reference image)
verification OK: wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:26.697 -01:59:01.08 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits (1st new image)
verification OK: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:48.286 -02:01:04.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:26.697 -01:59:01.08
Second-epoch image center 18:51:48.286 -02:01:04.81
Angular distance between the image centers 0.0962 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits (2nd new image)
verification OK: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:51.603 -02:00:15.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:26.697 -01:59:01.08
Second-epoch image center 18:51:51.603 -02:00:15.36
Angular distance between the image centers 0.1057 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:48.286 -02:01:04.81
Second-epoch second image center 18:51:51.603 -02:00:15.36
Angular distance between the image centers 0.01948 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/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits &> /tmp/tmp.V72ERhEMZj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits &> /tmp/tmp.MXj0usL3GZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits &> /tmp/tmp.FisfCQOQxm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits &> /tmp/tmp.oO1u9x6o3L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.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_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits and wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.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_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits and wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat
Found non-empty wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits and wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat
The reference image (wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat) found
'wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat' -> 'wcsmag.cat'
Read 14325 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 275.0070 to 290.7498 deg, Dec -7.2514 to +3.2826 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 275.0070 to 290.7498 deg, Dec -7.2514 to 3.2826 deg
Loaded 9410 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): 7025 out of 7466 total matches.
Matched with Tycho-2 7466 out of 14325 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.722900
a=0.000000 b=1.000000 c=22.722900
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.75
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.75
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 14325 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 275.0070 to 290.7498 deg, Dec -7.2514 to +3.2826 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 275.0070 to 290.7498 deg, Dec -7.2514 to 3.2826 deg
Loaded 9410 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): 7025 out of 7466 total matches.
Matched with Tycho-2 7466 out of 14325 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits -> calib.txt_param_ref_wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits (aperture=6.3)
Read 14138 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9988 to 290.7529 deg, Dec -7.2648 to +3.2822 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 274.9988 to 290.7529 deg, Dec -7.2648 to 3.2822 deg
Loaded 9437 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): 6996 out of 7464 total matches.
Matched with Tycho-2 7464 out of 14138 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits -> calib.txt_param_ref_wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
2.4 pix Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
2.4 pix fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
2.4 pix fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
2.4 pix wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
2.4 pix wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
Limiting magnitude estimates:
14.8 mag. Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
14.7 mag. Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
13.8 mag. fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
13.8 mag. fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.V72ERhEMZj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits' -> 'wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1242, passed=14325
Got 14325 stars (including 13071 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat
util/solve_plate_with_UCAC5 got 14325 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 14007 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 14005 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 14005 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits N_match=949 sigma_overall_arcsec=0.609 sigma_q1_arcsec=0.490 sigma_q2_arcsec=0.746 sigma_q3_arcsec=0.514 sigma_q4_arcsec=0.625 n_q1=189 n_q2=276 n_q3=192 n_q4=292 worst_quadrant_to_overall_ratio=1.225
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits -region wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.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.MXj0usL3GZ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits' -> 'wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1241, passed=14138
Got 14138 stars (including 12882 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat
util/solve_plate_with_UCAC5 got 14138 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 13841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 13842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 13842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits N_match=948 sigma_overall_arcsec=0.615 sigma_q1_arcsec=0.461 sigma_q2_arcsec=0.768 sigma_q3_arcsec=0.602 sigma_q4_arcsec=0.612 n_q1=186 n_q2=278 n_q3=189 n_q4=295 worst_quadrant_to_overall_ratio=1.249
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits -region wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.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.FisfCQOQxm (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_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.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_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=592, passed=5913
Got 5913 stars (including 5315 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat
util/solve_plate_with_UCAC5 got 5913 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits N_match=946 sigma_overall_arcsec=0.641 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.735 sigma_q3_arcsec=0.603 sigma_q4_arcsec=0.962 n_q1=280 n_q2=228 n_q3=230 n_q4=208 worst_quadrant_to_overall_ratio=1.501
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits -region wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.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.oO1u9x6o3L (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_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.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_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=448, passed=5453
Got 5453 stars (including 5001 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 5453 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits N_match=944 sigma_overall_arcsec=0.623 sigma_q1_arcsec=0.488 sigma_q2_arcsec=0.692 sigma_q3_arcsec=0.528 sigma_q4_arcsec=0.997 n_q1=285 n_q2=228 n_q3=229 n_q4=202 worst_quadrant_to_overall_ratio=1.601
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits -region wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits sigma_overall=0.609 worst_q_ratio=1.225
ref2=Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits sigma_overall=0.615 worst_q_ratio=1.249
new1=fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits sigma_overall=0.641 worst_q_ratio=1.501
new2=fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits sigma_overall=0.623 worst_q_ratio=1.601
reference average sigma_overall=0.612 worst_q_ratio=1.237
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122_astrometric_residuals.png (949 matched stars from wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205_astrometric_residuals.png (948 matched stars from wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257_astrometric_residuals.png (946 matched stars from wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.63 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258_astrometric_residuals.png (944 matched stars from wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.61 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits'
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:51:01.76 -06:15:34.3: 10.95 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:51:01.76 -06:15:34.3: 10.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.94 +/- 0.03
Forced photometry filter REJECTED candidate at 18:51:01.76 -06:15:34.3: ref_mag=10.94 +/- 0.03 new_mean_mag=10.5321 delta=0.40 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21277_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 21277_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21643_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 21643_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:51:02.53 -06:14:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21882_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 21882_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:51:03.87 -06:13:54.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits exists and is non-empty
wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits (1st reference image)
verification OK: wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:26.697 -01:59:01.08 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits (1st new image)
verification OK: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:48.286 -02:01:04.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:26.697 -01:59:01.08
Second-epoch image center 18:51:48.286 -02:01:04.81
Angular distance between the image centers 0.0962 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits (2nd new image)
verification OK: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:51.603 -02:00:15.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:26.697 -01:59:01.08
Second-epoch image center 18:51:51.603 -02:00:15.36
Angular distance between the image centers 0.1057 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:48.286 -02:01:04.81
Second-epoch second image center 18:51:51.603 -02:00:15.36
Angular distance between the image centers 0.01948 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/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits &> /tmp/tmp.q0Ny56nTf8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits &> /tmp/tmp.t3y2WTieMa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits &> /tmp/tmp.5jqGzP0MZG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits &> /tmp/tmp.0P3fOAbw1k
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.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_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits and wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.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_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits and wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat
Found non-empty wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits and wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat
The reference image (wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat) found
'wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat' -> 'wcsmag.cat'
Read 148413 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 275.0028 to 290.7497 deg, Dec -7.2529 to +3.2886 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 275.0028 to 290.7497 deg, Dec -7.2529 to 3.2886 deg
Loaded 9416 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): 6295 out of 8220 total matches.
Matched with Tycho-2 8220 out of 148413 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.524400
a=0.000000 b=1.000000 c=22.524400
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.88
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.88
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 148413 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 275.0028 to 290.7497 deg, Dec -7.2529 to +3.2886 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 275.0028 to 290.7497 deg, Dec -7.2529 to 3.2886 deg
Loaded 9416 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): 6295 out of 8220 total matches.
Matched with Tycho-2 8220 out of 148413 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits -> calib.txt_param_ref_wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits (aperture=4.5)
Read 150207 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9984 to 290.7583 deg, Dec -7.2661 to +3.2823 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 274.9984 to 290.7583 deg, Dec -7.2661 to 3.2823 deg
Loaded 9443 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): 6275 out of 8241 total matches.
Matched with Tycho-2 8241 out of 150207 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits -> calib.txt_param_ref_wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 60 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
2.1 pix Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
2.2 pix fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
2.2 pix fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
2.2 pix wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
2.1 pix wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
Limiting magnitude estimates:
14.9 mag. Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
14.9 mag. Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
14.0 mag. fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
13.9 mag. fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.4 (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.q0Ny56nTf8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits' -> 'wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=18535, passed=148397
Got 148397 stars (including 129670 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat
util/solve_plate_with_UCAC5 got 148397 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 146157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 146158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 146158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits N_match=948 sigma_overall_arcsec=0.593 sigma_q1_arcsec=0.480 sigma_q2_arcsec=0.706 sigma_q3_arcsec=0.510 sigma_q4_arcsec=0.597 n_q1=189 n_q2=271 n_q3=203 n_q4=285 worst_quadrant_to_overall_ratio=1.190
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits -region wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.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.t3y2WTieMa (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits' -> 'wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat corresponding to the image wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=19074, passed=150190
Got 150190 stars (including 130922 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat
util/solve_plate_with_UCAC5 got 150190 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 147558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 147559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 147559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits N_match=948 sigma_overall_arcsec=0.592 sigma_q1_arcsec=0.497 sigma_q2_arcsec=0.680 sigma_q3_arcsec=0.590 sigma_q4_arcsec=0.625 n_q1=190 n_q2=273 n_q3=194 n_q4=291 worst_quadrant_to_overall_ratio=1.148
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits -region wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.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.5jqGzP0MZG (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_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.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_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=4330, passed=68376
Got 68376 stars (including 63920 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat
util/solve_plate_with_UCAC5 got 68376 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 66960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.2)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 66961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 66960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits N_match=944 sigma_overall_arcsec=0.627 sigma_q1_arcsec=0.511 sigma_q2_arcsec=0.678 sigma_q3_arcsec=0.612 sigma_q4_arcsec=0.974 n_q1=294 n_q2=210 n_q3=256 n_q4=184 worst_quadrant_to_overall_ratio=1.555
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits -region wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.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.0P3fOAbw1k (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_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.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_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=3673, passed=62687
Got 62687 stars (including 58933 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 62687 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 61418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 61413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 61412 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits N_match=944 sigma_overall_arcsec=0.597 sigma_q1_arcsec=0.503 sigma_q2_arcsec=0.649 sigma_q3_arcsec=0.522 sigma_q4_arcsec=0.993 n_q1=298 n_q2=211 n_q3=253 n_q4=182 worst_quadrant_to_overall_ratio=1.664
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits -region wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.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_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.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_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-40-11_20.00sec_5.00C_LIGHT_0257.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.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_2026-06-10_CI_Aql-03-Q2b1x1_060020_TTUQ2b1x1_2227004_7Lqxgcs9/wcs_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258.fits
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:08:06.31 +00:51:12.3: 13.13 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:36:21.74 -06:05:15.4: 12.99 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:58:23.84 -06:05:51.1: 13.06 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:04:13.42 -04:49:20.7: 13.53 +/- 0.06 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:57:19.02 -00:47:29.3: 13.16 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:01:54.60 -01:49:34.1: 13.21 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:46:23.25 -05:04:38.1: 12.68 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:59:28.84 -05:53:15.7: 13.01 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:05:58.21 -06:04:51.8: 12.82 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:58:23.84 -06:05:51.1: 13.10 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:57:19.02 -00:47:29.3: 13.16 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:08:06.31 +00:51:12.3: 13.24 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:01:54.60 -01:49:34.1: 13.34 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:36:21.74 -06:05:15.4: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:04:13.42 -04:49:20.7: 13.48 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter REJECTED candidate at 18:57:19.02 -00:47:29.3: ref_mag=13.16 +/- 0.03 new_mean_mag=13.2231 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:58:23.84 -06:05:51.1: ref_mag=13.08 +/- 0.03 new_mean_mag=13.2865 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:08:06.31 +00:51:12.3: ref_mag=13.18 +/- 0.03 new_mean_mag=13.7120 delta=-0.54 (need > 0.90)
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:46:23.25 -05:04:38.1: 12.73 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 19:01:54.60 -01:49:34.1: ref_mag=13.27 +/- 0.03 new_mean_mag=13.4706 delta=-0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:36:21.74 -06:05:15.4: ref_mag=12.98 +/- 0.03 new_mean_mag=13.0939 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry filter REJECTED candidate at 19:04:13.42 -04:49:20.7: ref_mag=13.51 +/- 0.04 new_mean_mag=13.7834 delta=-0.28 (need > 0.90)
Forced photometry reference-image weighted average: 12.70 +/- 0.03
Forced photometry filter REJECTED candidate at 18:46:23.25 -05:04:38.1: ref_mag=12.70 +/- 0.03 new_mean_mag=12.9042 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:04:32.05 -06:14:02.8: 12.35 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:05:58.21 -06:04:51.8: 12.87 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:59:28.84 -05:53:15.7: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.03
Forced photometry filter REJECTED candidate at 19:05:58.21 -06:04:51.8: ref_mag=12.84 +/- 0.03 new_mean_mag=12.9398 delta=-0.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.01 +/- 0.03
Forced photometry filter REJECTED candidate at 18:59:28.84 -05:53:15.7: ref_mag=13.01 +/- 0.03 new_mean_mag=13.0094 delta=0.00 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:04:32.05 -06:14:02.8: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Forced photometry filter REJECTED candidate at 19:04:32.05 -06:14:02.8: ref_mag=12.35 +/- 0.02 new_mean_mag=12.5937 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:51:04.82 -00:03:59.2: 12.49 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:40:46.69 -04:14:38.6: 13.00 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:36:26.31 -04:43:57.4: 13.39 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:51:04.82 -00:03:59.2: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter REJECTED candidate at 18:51:04.82 -00:03:59.2: ref_mag=12.48 +/- 0.01 new_mean_mag=12.3712 delta=0.11 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:40:46.69 -04:14:38.6: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter REJECTED candidate at 18:40:46.69 -04:14:38.6: ref_mag=13.00 +/- 0.02 new_mean_mag=12.3760 delta=0.63 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:55:47.76 -00:45:13.6: 12.86 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:36:26.31 -04:43:57.4: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.04
Forced photometry filter REJECTED candidate at 18:36:26.31 -04:43:57.4: ref_mag=13.42 +/- 0.04 new_mean_mag=12.7642 delta=0.65 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:55:47.76 -00:45:13.6: 12.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.03
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:07:26.17 -01:09:22.7: 13.12 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 18:55:47.76 -00:45:13.6: ref_mag=12.88 +/- 0.03 new_mean_mag=12.9760 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:36:35.64 -03:04:03.2: 12.97 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:09:13.19 -06:03:58.2: 13.16 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:51:59.46 -05:08:50.2: 13.15 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:00:28.50 -05:22:15.2: 13.20 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:07:26.17 -01:09:22.7: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter REJECTED candidate at 19:07:26.17 -01:09:22.7: ref_mag=13.12 +/- 0.03 new_mean_mag=13.1257 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:36:35.64 -03:04:03.2: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Forced photometry filter REJECTED candidate at 18:36:35.64 -03:04:03.2: ref_mag=12.98 +/- 0.03 new_mean_mag=12.9859 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:08:57.79 +01:20:22.9: 13.14 +/- 0.06 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:09:13.19 -06:03:58.2: 13.13 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:07:47.35 +01:12:39.6: 13.23 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Forced photometry filter REJECTED candidate at 19:09:13.19 -06:03:58.2: ref_mag=13.14 +/- 0.03 new_mean_mag=13.1817 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:51:59.46 -05:08:50.2: 13.29 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.04
Forced photometry filter REJECTED candidate at 18:51:59.46 -05:08:50.2: ref_mag=13.21 +/- 0.04 new_mean_mag=13.1251 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:52:25.13 -02:40:10.6: 13.23 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:00:28.50 -05:22:15.2: 13.30 +/- 0.06 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 19:04:22.97 +00:17:57.3: 13.38 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.04
Forced photometry filter REJECTED candidate at 19:00:28.50 -05:22:15.2: ref_mag=13.24 +/- 0.04 new_mean_mag=13.2108 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:08:57.79 +01:20:22.9: 13.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.04
Forced photometry filter REJECTED candidate at 19:08:57.79 +01:20:22.9: ref_mag=13.10 +/- 0.04 new_mean_mag=13.2362 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:07:47.35 +01:12:39.6: 13.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.04
Forced photometry filter REJECTED candidate at 19:07:47.35 +01:12:39.6: ref_mag=13.24 +/- 0.04 new_mean_mag=13.2793 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:52:25.13 -02:40:10.6: 13.28 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Forced photometry filter REJECTED candidate at 18:52:25.13 -02:40:10.6: ref_mag=13.26 +/- 0.03 new_mean_mag=13.2638 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 19:04:22.97 +00:17:57.3: 13.43 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.05
Forced photometry filter REJECTED candidate at 19:04:22.97 +00:17:57.3: ref_mag=13.40 +/- 0.05 new_mean_mag=13.4383 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:51:14.89 -04:43:04.6: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:51:14.89 -04:43:04.6: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:40:48.63 -05:47:47.8: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:42:08.51 -02:45:11.3: 13.26 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:42:08.51 -02:45:11.3: 13.27 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:40:48.63 -05:47:47.8: 15.02 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Forced photometry filter KEPT candidate at 18:42:08.51 -02:45:11.3: ref_mag=13.26 +/- 0.03 new_mean_mag=12.2306 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:34:24.86 +01:27:27.5: 13.78 +/- 0.07 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-15_03-45-29_20.00sec_0.00C_LIGHT_0122.fits at 18:40:53.23 -02:38:16.3: 13.49 +/- 0.06 detection
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:34:24.86 +01:27:27.5: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.05
Forced photometry filter KEPT candidate at 18:34:24.86 +01:27:27.5: ref_mag=13.81 +/- 0.05 new_mean_mag=12.7268 delta=1.09 (need > 0.90)
Forced photometry on wcs_Aql-03-Q2b1x1_2026-05-16_02-59-02_20.00sec_-0.00C_LIGHT_0205.fits at 18:40:53.23 -02:38:16.3: 13.59 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry filter KEPT candidate at 18:40:53.23 -02:38:16.3: ref_mag=13.53 +/- 0.04 new_mean_mag=12.6230 delta=0.91 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out28594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out73602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out109868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72096.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 171254_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171254_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 171263_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171263_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 171264_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171264_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 171280_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171280_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 171291_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171291_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:58:45.99 -00:09:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171292_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171292_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 171297_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171297_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 171303_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171303_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:07:06.60 -03:20:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171305_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171305_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:49:09.40 -06:03:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171307_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171307_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 171316_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171316_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 171323_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171323_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:08:05.51 -00:54:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171325_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171325_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 171334_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 171334_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 173795_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 173795_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:47:01.81 -04:44:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174193_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 174193_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:01:33.47 -05:43:08.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 174255_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 174255_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:04:20.72 -05:42:46.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 174846_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 174846_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:02:58.78 -03:43:11.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 176177_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 176177_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 176806_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 176806_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 178507_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 178507_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:40:42.03 -04:29:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178753_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 178753_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:02:58.41 -03:40:40.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 178977_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 178977_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:49:46.99 -05:54:33.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 179377_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 179377_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:04:59.20 +01:36:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 179473_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 179473_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 179528_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 179528_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:47:27.18 -05:43:54.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181081_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 181081_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 181129_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 181129_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:38:28.79 -03:11:33.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181319_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 181319_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:56:56.69 -00:47:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181520_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 181520_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:07:42.74 +02:15:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181789_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 181789_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:56:11.33 -00:29:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182165_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 182165_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:06:07.14 -04:53:36.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 182224_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 182224_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 182704_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 182704_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 182865_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 182865_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 183223_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 183223_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 183502_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 183502_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 183555_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 183555_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 183558_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 183558_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:07:35.83 -04:56:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184007_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 184007_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:00:48.68 +01:23:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184472_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 184472_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 184618_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 184618_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 185045_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 185045_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 185353_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 185353_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:38:09.02 -04:29:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185491_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 185491_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
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Considering the candidate 186558_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 186558_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:39:04.52 +01:41:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187354_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 187354_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 188889_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 188889_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:07:48.01 +00:07:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190063_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
Preparing report for the candidate 190063_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
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Considering the candidate 191080_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 191080_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:00:39.06 -00:14:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25180_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 25180_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:56:48.60 -05:56:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72096_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
Preparing report for the candidate 72096_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
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Considering the candidate 28594_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 28594_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:40:48.63 -05:47:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.658 4253471937669952768 280.20221617112 -05.79682689427 12.9383 10.8958 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 164732_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 164732_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:39:52.37 -04:23:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22172_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 22172_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:44:53.08 -06:07:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97161_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 97161_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:34:15.09 -00:58:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69660_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 69660_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 18:36:42.32 -02:57:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109868_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
Preparing report for the candidate 109868_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
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Considering the candidate 58274_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 58274_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks
**** FOUND 19:08:04.37 -03:50:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73602_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258
The candidate 73602_fd_Aql-03-Q2b1x1_2026-06-10_05-41-14_20.00sec_5.00C_LIGHT_0258 did not pass the final checks