This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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 03 26.1093* 04 01 56.58 +02 11 37.4 12.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.6093,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1093 12.66CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:01:56.58 +02:11:37.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20_00sec_-14_90C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20_00sec_-10_00C_LIGHT_0287_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20_00sec_-14_90C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20_00sec_-10_00C_LIGHT_0286_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20_00sec_-14_90C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20_00sec_-10_00C_LIGHT_0287_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20_00sec_-14_90C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20_00sec_-10_00C_LIGHT_0286_fits__*pix.png animation_v2.gif
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 03 26.1093* 04 33 44.74 +00 01 35.0 9.4 U Eri 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BD Eri,2461125.6093,9.38,0.05,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
BD Eri 20260326.1093 9.38CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:44.74 +00:01:35.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20_00sec_-14_90C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20_00sec_-10_00C_LIGHT_0287_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20_00sec_-14_90C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20_00sec_-10_00C_LIGHT_0286_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20_00sec_-14_90C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20_00sec_-10_00C_LIGHT_0287_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20_00sec_-14_90C_LIGHT_0135_fits__*pix.png resample_wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20_00sec_-10_00C_LIGHT_0286_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.67043058 09.01.2026 04:05:15.202 /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
First image: 2461049.67043058 09.01.2026 04:05:15.202 /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
Last image: 2461125.60957240 26.03.2026 02:37:37.055 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
JD time system (TT/UTC/UNKNOWN): UTC
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: 3 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): 7559
Objects passed selection criteria: 7533
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 6118.5
Average stars matched: 5989.25 (97.8876 %)
Memory usage VmPeak: 114112 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 21:46:52 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: 2461049.67043058 09.01.2026 04:05:15.202 /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
First image: 2461049.67043058 09.01.2026 04:05:15.202 /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
Last image: 2461125.60957240 26.03.2026 02:37:37.055 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 78
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 16 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): 44662
Objects passed selection criteria: 44572
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 37224.8
Average stars matched: 36139.8 (97.0853 %)
Memory usage VmPeak: 148220 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 21:47:40 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/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
SExtractor catalog cache: saved Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat to cache
SExtractor catalog cache: saved Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.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/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.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: 2461125.60903924
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits exists and is non-empty
Saving wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits to local_wcs_cache/
'wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits' -> 'local_wcs_cache/wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits'
wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits exists and is non-empty
Saving wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits to local_wcs_cache/
'wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits' -> 'local_wcs_cache/wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits'
wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits exists and is non-empty
Saving wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits to local_wcs_cache/
'wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits' -> 'local_wcs_cache/wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits'
wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits exists and is non-empty
Saving wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits to local_wcs_cache/
'wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits' -> 'local_wcs_cache/wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:17:09.540 -01:59:58.56
Second-epoch image center 04:17:17.454 -01:58:20.86
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:17:09.540 -01:59:58.56
Second-epoch image center 04:17:17.524 -01:58:43.05
Angular distance between the image centers 0.04 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 04:17:17.454 -01:58:20.86
Second-epoch second image center 04:17:17.524 -01:58:43.05
Angular distance between the image centers 0.00617 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/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits &> /tmp/tmp.De34C35V0W
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits &> /tmp/tmp.5y8wJhv1HE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits &> /tmp/tmp.8vLWM3Rdrk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits &> /tmp/tmp.2Mwpgmn95N
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
Calibrating the magnitude scale
Found non-empty wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.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_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits and wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits and wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat
Found non-empty wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits and wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat
The reference image (wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits) and catalog (wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat) found
'wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5013 out of 9074 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.900759
a=0.000000 b=1.000000 c=22.900759
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
2.0 pix Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
2.4 pix fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
2.5 pix fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
Limiting magnitude estimates:
15.3 mag. Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
15.3 mag. Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
14.2 mag. fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
14.2 mag. fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.4 (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.De34C35V0W (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits' -> 'wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
WCS_IMAGE_NAME=wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
WCS-calibrated image found: wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
Checking if the catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat corresponding to the image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits alredy exist and is non-empty...
Catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat corresponding to the image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
WCS catalog name: wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=748, passed=9074
Got 9074 stars (including 8321 good ones) from the SExtractor catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat
util/solve_plate_with_UCAC5 got 9074 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits -region wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5y8wJhv1HE (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits' -> 'wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
WCS_IMAGE_NAME=wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
WCS-calibrated image found: wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
Checking if the catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat corresponding to the image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits alredy exist and is non-empty...
Catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat corresponding to the image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
WCS catalog name: wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=759, passed=9104
Got 9104 stars (including 8332 good ones) from the SExtractor catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat
util/solve_plate_with_UCAC5 got 9104 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits -region wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8vLWM3Rdrk (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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
WCS_IMAGE_NAME=wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
WCS-calibrated image found: wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
Checking if the catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat corresponding to the image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat corresponding to the image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
WCS catalog name: wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=339, passed=4821
Got 4821 stars (including 4482 good ones) from the SExtractor catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat
util/solve_plate_with_UCAC5 got 4821 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits -region wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2Mwpgmn95N (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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
WCS_IMAGE_NAME=wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
WCS-calibrated image found: wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
Checking if the catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat corresponding to the image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat corresponding to the image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
WCS catalog name: wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=332, passed=4857
Got 4857 stars (including 4523 good ones) from the SExtractor catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat
util/solve_plate_with_UCAC5 got 4857 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits -region wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits'
Saving fully-calibrated image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits'
Saving fully-calibrated image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits'
Saving fully-calibrated image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits'
Preparing the HTML report for the field Eri-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Eri-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
SExtractor catalog cache: saved Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat to cache
SExtractor catalog cache: saved Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
Creating symlink local_wcs_cache/wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
Creating symlink local_wcs_cache/wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
Creating symlink local_wcs_cache/wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.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_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits exists and is non-empty
wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits exists and is non-empty
wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits exists and is non-empty
wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:17:09.540 -01:59:58.56
Second-epoch image center 04:17:17.454 -01:58:20.86
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:17:09.540 -01:59:58.56
Second-epoch image center 04:17:17.524 -01:58:43.05
Angular distance between the image centers 0.04 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 04:17:17.454 -01:58:20.86
Second-epoch second image center 04:17:17.524 -01:58:43.05
Angular distance between the image centers 0.00617 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/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits &> /tmp/tmp.VCt7uNvYwZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits &> /tmp/tmp.OiKbW0oprW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits &> /tmp/tmp.P2nma4lR38
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits &> /tmp/tmp.LHl7CBZjJK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
Calibrating the magnitude scale
Found non-empty wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.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_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits and wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits and wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat
Found non-empty wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits and wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat
The reference image (wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits) and catalog (wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat) found
'wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5077 out of 53209 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.779496
a=0.000000 b=1.000000 c=22.779496
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
1.9 pix Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
2.2 pix fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
2.3 pix fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
Limiting magnitude estimates:
15.4 mag. Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
15.4 mag. Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
14.4 mag. fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
14.4 mag. fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.VCt7uNvYwZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits' -> 'wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
WCS_IMAGE_NAME=wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
WCS-calibrated image found: wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
Checking if the catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat corresponding to the image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits alredy exist and is non-empty...
Catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat corresponding to the image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
WCS catalog name: wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2903, passed=53198
Got 53198 stars (including 50212 good ones) from the SExtractor catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat
util/solve_plate_with_UCAC5 got 53198 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits -region wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OiKbW0oprW (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits' -> 'wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
WCS_IMAGE_NAME=wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
WCS-calibrated image found: wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
Checking if the catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat corresponding to the image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits alredy exist and is non-empty...
Catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat corresponding to the image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
WCS catalog name: wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2925, passed=53486
Got 53486 stars (including 50465 good ones) from the SExtractor catalog wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat
util/solve_plate_with_UCAC5 got 53486 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits -region wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.P2nma4lR38 (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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
WCS_IMAGE_NAME=wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
WCS-calibrated image found: wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
Checking if the catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat corresponding to the image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat corresponding to the image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
WCS catalog name: wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1293, passed=29019
Got 29019 stars (including 27686 good ones) from the SExtractor catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat
util/solve_plate_with_UCAC5 got 29019 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits -region wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LHl7CBZjJK (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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
WCS_IMAGE_NAME=wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
WCS-calibrated image found: wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
Checking if the catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat corresponding to the image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat corresponding to the image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
WCS catalog name: wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1178, passed=28529
Got 28529 stars (including 27314 good ones) from the SExtractor catalog wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat
util/solve_plate_with_UCAC5 got 28529 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits -region wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/wcs_Eri-02-Q2b1x1_2026-01-08_22-05-15_20.00sec_-14.90C_LIGHT_0135.fits
Saving fully-calibrated image wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/wcs_Eri-02-Q2b1x1_2026-01-08_22-05-55_20.00sec_-15.00C_LIGHT_0136.fits
Saving fully-calibrated image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-36-50_20.00sec_-10.00C_LIGHT_0286.fits
Saving fully-calibrated image wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.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_2026-03-25_CI_Eri-02-Q2b1x1_214304_TTUQ2b1x1_8768_ZYEqLLVd/wcs_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287.fits
Preparing the HTML report for the field Eri-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out67017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out15612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67104.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 67017_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67017_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:18:07.14 +00:37:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.893 3255625484278214272 064.52951736938 +00.62919760516 13.7394 13.1911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67023_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67023_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:26:35.28 -00:48:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 0.191 3206412237171409920 066.64699049893 -00.80521875347 11.6052 11.1562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67067_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67067_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 67086_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67086_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 67104_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
Preparing report for the candidate 67104_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
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Considering the candidate 67126_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67126_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 67145_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67145_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 67153_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67153_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:25:49.93 +01:07:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.632 3278979862870010496 066.45760424315 +01.12039674983 13.3858 12.8626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67172_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67172_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 67175_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67175_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 67179_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67179_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 03:55:06.45 -04:57:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.826 3246147934565436288 058.77669651474 -04.95932731314 13.0469 12.5537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67180_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67180_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:40:17.25 +01:14:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.614 3231101530255584768 070.07184786803 +01.24377460030 13.9275 13.3372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67190_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67190_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:35:07.93 -04:48:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.877 3201261437513241984 068.78229250013 -04.81503616248 13.4958 12.8131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67200_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67200_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 67208_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67208_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:21:07.76 +01:12:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.972 3255763610426071296 065.28267381203 +01.21465126573 13.3953 12.8577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67213_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67213_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:01:36.00 -01:31:29.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 67232_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67232_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 67237_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67237_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:33:41.99 -01:51:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.339 3205385224592161664 068.42502249988 -01.85329132451 13.3896 12.9378 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67242_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67242_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:20:20.11 -02:38:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.473 3205742497152821120 065.08435852631 -02.64988897735 13.6052 12.8325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67267_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67267_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 67271_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67271_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:20:26.35 -01:57:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.460 3253888496426194688 065.10963945260 -01.96437412786 13.7745 13.3132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67273_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67273_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:15:02.61 -00:58:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.408 3254256557943292800 063.76098789372 -00.98153744115 13.2482 12.1799 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67287_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67287_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 67290_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67290_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 67313_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67313_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:12:14.10 +00:43:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.315 3255498353247192704 063.05871300235 +00.71713495388 13.8192 13.1177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67314_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67314_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 67317_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67317_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 67324_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67324_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 67325_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67325_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:21:16.81 -01:50:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.581 3253897052001028608 065.31993192704 -01.83438143133 13.6616 13.3664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67330_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67330_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 67349_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67349_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 67355_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67355_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 67373_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67373_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 67375_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67375_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 67376_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67376_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 67382_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67382_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 67388_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67388_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 67403_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67403_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 67407_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67407_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 67416_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67416_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 67420_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67420_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 67423_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67423_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 67426_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67426_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
**** FOUND 04:21:18.03 -01:50:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.006 3253897052001028736 065.32496674679 -01.83873030097 14.2113 13.6823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67431_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67431_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 67446_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67446_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 67449_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67449_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 67450_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67450_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 67461_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67461_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 67464_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67464_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 67470_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67470_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 67482_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287
The candidate 67482_fd_Eri-02-Q2b1x1_2026-03-25_21-37-37_20.00sec_-10.00C_LIGHT_0287 did not pass the final checks