This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax
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!
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
GDS_J1854007-054756,2461128.8724,12.73,0.05,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
GDS_J1854007-054756 20260329.3724 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:54:01.97 -05:47:58.5 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3724 2461128.8724 12.84 19:12:02.41 +00:53:33.6
36.08141 -4.17388 galactic Aql Second-epoch detections are separated by 5.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J191204.01+005345.7 | 19:12:04.01 +00:53:45.7 (Gaia DR3) | SR (local) | 2458921.64400 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191204.01+005345.7,2461128.8724,12.84,0.05,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
ASASSN-V J191204.01+005345.7 20260329.3724 12.84CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:12:02.41 +00:53:33.6 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
Gaia DR3 4253409883961723136,2461128.8724,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4253409883961723136 20260329.3724 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:43:12.29 -06:06:09.0 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
Pej 006,2461128.8724,12.90,0.05,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
Pej 006 20260329.3724 12.90CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:04:01.07 -03:05:12.8 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
FASTT 1360,2461128.8724,12.58,0.05,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
FASTT 1360 20260329.3724 12.58CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:51:53.69 -00:58:45.6 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
V1551 Aql,2461128.8724,12.12,0.05,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
V1551 Aql 20260329.3724 12.12CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:52:35.86 -03:12:17.5 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
NSVS 13966472,2461128.8724,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13966472 20260329.3724 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:58:15.30 -03:00:01.9 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
NSVS 13935563,2461128.8724,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13935563 20260329.3724 12.88CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:34:21.22 -05:53:18.0 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
NSV 11681,2461128.8724,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 11681 20260329.3724 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:02:52.84 -05:50:29.5 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
2MASS J19073891-0558568,2461128.8724,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J19073891-0558568 20260329.3724 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:07:38.70 -05:58:54.1 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3724 2461128.8724 11.76 19:14:45.03 -01:08:32.0
34.57623 -5.70724 galactic Aql Second-epoch detections are separated by 0.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J288.6906-01.1483 | 19:14:45.37 -01:08:30.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J288.6906-01.1483,2461128.8724,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.6906-01.1483 20260329.3724 11.76CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:14:45.03 -01:08:32.0 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
NSVS 13967220,2461128.8724,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13967220 20260329.3724 12.65CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:58:43.01 -02:16:38.9 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
NSVS 13953120,2461128.8724,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13953120 20260329.3724 12.94CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:48:41.09 -05:27:55.3 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
NSVS J1908596-030148,2461128.8724,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1908596-030148 20260329.3724 12.04CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:08:59.33 -03:01:48.0 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
NSVS J1913248+011811,2461128.8724,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1913248+011811 20260329.3724 12.54CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:13:24.79 +01:18:08.5 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
NSVS J1909126-054849,2461128.8724,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1909126-054849 20260329.3724 12.62CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:09:12.32 -05:48:46.9 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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!
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
GDS_J1845447-051418,2461128.8724,12.54,0.05,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
GDS_J1845447-051418 20260329.3724 12.54CV 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:45:44.59 -05:14:19.0 ;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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20_00sec_-15_00C_LIGHT_0328_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20_00sec_-14_90C_LIGHT_0051_fits__*pix.png resample_wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20_00sec_-15_00C_LIGHT_0327_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: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
First image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Last image: 2461128.87271863 29.03.2026 08:56:32.890 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.06
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 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): 9791
Objects passed selection criteria: 9766
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 7836.5
Average stars matched: 7615 (97.1735 %)
Memory usage VmPeak: 116676 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 Sun Mar 29 04:00:18 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: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
First image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Last image: 2461128.87271863 29.03.2026 08:56:32.890 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 111
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 25 seconds
Number of parallel threads: 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): 115286
Objects passed selection criteria: 115015
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 88613.8
Average stars matched: 84778.8 (95.6722 %)
Memory usage VmPeak: 1890484 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 Sun Mar 29 04:02:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.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: 2461128.87212460
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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits'
wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.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 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:38.858 -02:00:10.90
Angular distance between the image centers 0.06 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 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:36.358 -02:00:07.82
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:38.858 -02:00:10.90
Second-epoch second image center 18:51:36.358 -02:00:07.82
Angular distance between the image centers 0.01044 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits &> /tmp/tmp.C3NwH4l7zL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits &> /tmp/tmp.uEy9lFa15T
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits &> /tmp/tmp.hXIRGSdRUI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits &> /tmp/tmp.F06e95vfC2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
The reference image (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat) found
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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 7408 out of 13310 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.858998
a=0.000000 b=1.000000 c=22.858998
From vast_summary.log: estimated ref. image limiting mag.: -8.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.80
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
2.3 pix Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
2.9 pix fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
2.9 pix fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
Limiting magnitude estimates:
14.8 mag. Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
14.8 mag. Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
13.8 mag. fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
13.9 mag. fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.C3NwH4l7zL (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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1253, passed=13310
Got 13310 stars (including 12037 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 13310 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 946 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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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.uEy9lFa15T (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/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1265, passed=13307
Got 13307 stars (including 12019 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 13307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 944 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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.hXIRGSdRUI (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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=373, passed=5910
Got 5910 stars (including 5529 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat
util/solve_plate_with_UCAC5 got 5910 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 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 942 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.71"
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits -region wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.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.F06e95vfC2 (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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=378, passed=5958
Got 5958 stars (including 5573 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat
util/solve_plate_with_UCAC5 got 5958 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 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 941 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: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits -region wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
Saving fully-calibrated image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits'
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20855_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 20855_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:56:09.20 -00:28:33.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits exists and is non-empty
wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.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 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:38.858 -02:00:10.90
Angular distance between the image centers 0.06 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 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:36.358 -02:00:07.82
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:38.858 -02:00:10.90
Second-epoch second image center 18:51:36.358 -02:00:07.82
Angular distance between the image centers 0.01044 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits &> /tmp/tmp.cekF4EbZIM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits &> /tmp/tmp.gbLPf11cjB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits &> /tmp/tmp.e1aoZtqQJT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits &> /tmp/tmp.xxVJ5kAmhp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
The reference image (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat) found
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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 8387 out of 153764 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.669636
a=0.000000 b=1.000000 c=22.669636
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 62 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
2.1 pix Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
2.5 pix fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
2.5 pix fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
Limiting magnitude estimates:
14.9 mag. Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
14.9 mag. Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
13.9 mag. fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
13.9 mag. fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (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.cekF4EbZIM (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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=17867, passed=153743
Got 153743 stars (including 135593 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 153743 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 946 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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.gbLPf11cjB (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/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=18180, passed=153307
Got 153307 stars (including 134827 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 153307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 941 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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.e1aoZtqQJT (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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3606, passed=53007
Got 53007 stars (including 49339 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat
util/solve_plate_with_UCAC5 got 53007 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 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 944 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: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits -region wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.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.xxVJ5kAmhp (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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=3731, passed=53812
Got 53812 stars (including 50016 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat
util/solve_plate_with_UCAC5 got 53812 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 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 942 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: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits -region wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Saving fully-calibrated image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-55-41_20.00sec_-15.00C_LIGHT_0327.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.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_2026-03-29_CI_Aql-03-Q2b1x1_035717_TTUQ2b1x1_406_1HG9BCax/wcs_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328.fits
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out165168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out73428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out83983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out178617.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out100368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84634.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 7s
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Considering the candidate 178602_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178602_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:15:18.29 +00:10:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 5.655 4264046971777875840 288.82771466420 +00.17666598158 12.2117 10.8061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178606_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178606_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:50:06.90 +01:20:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.453 4278988303971463424 282.52888286223 +01.34067445207 13.4412 12.7925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178608_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178608_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:59:56.14 -02:33:01.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178610_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178610_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:43:32.34 -01:39:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178617_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178617_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:40:32.50 -02:13:28.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 178624_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178624_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:36:22.25 -06:05:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 3.813 4256076474519927680 279.09301724523 -06.08370851706 13.1298 12.5718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178626_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 178626_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
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Considering the candidate 178627_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178627_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:03:50.22 -06:14:42.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
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Considering the candidate 178630_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 178630_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178632_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178632_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:05:34.23 -00:25:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178633_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 178633_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178634_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178634_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:13:37.23 -00:05:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178635_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178635_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:13:31.97 -02:28:05.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178638_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178638_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:08:05.68 -00:54:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 5.067 4262530088077004032 287.02288680174 -00.91082821919 12.4780 11.4616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178641_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178641_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:55:46.71 -00:39:00.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178651_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178651_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:14:36.56 -03:37:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 3.465 4212914733265314048 288.65317146228 -03.62647597308 11.6026 10.5327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178695_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178695_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:47:01.86 -04:44:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178715_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178715_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:02:58.67 -03:43:12.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 178719_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178719_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:15:48.02 -03:55:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178732_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178732_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:04:20.77 -05:42:45.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 178741_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178741_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:01:33.64 -05:43:09.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 178858_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178858_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:57:32.29 -06:14:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178860_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178860_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:47:27.31 -05:43:49.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 178865_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178865_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:07:37.27 +00:06:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178875_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178875_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:56:56.65 -00:47:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 4.868 4265348209484450048 284.23739066299 -00.78468183362 12.9189 12.4229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178885_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178885_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:07:43.98 -02:25:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178887_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178887_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:51:35.96 -05:18:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.695 4254835843150418304 282.89979101672 -05.30303101981 12.5564 11.3566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178897_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178897_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:15:46.46 -03:49:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 4.957 4212863464219546112 288.94469368398 -03.83212658891 12.4381 11.4672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178911_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178911_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:43:16.32 -00:57:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.288 4260193389672224384 280.81833121658 -00.96432036866 13.0253 11.9046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178932_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178932_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:16:01.62 -03:46:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.966 4212864185774723328 289.00783270417 -03.77079894454 12.1460 10.8813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178966_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 178966_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:52:05.03 -05:12:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.360 4254843956418818048 283.02133778286 -05.20538518183 11.9587 10.4337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166636_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 166636_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:15:59.24 -01:47:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74720_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 74720_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86878_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 86878_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:11:31.65 -02:05:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165162_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 165162_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:09:00.96 +00:21:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103890_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 103890_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73075_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 73075_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33038_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 33038_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:55:16.94 -05:47:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75955_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 75955_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31238_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 31238_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165675_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 165675_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:15:56.08 -02:17:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31780_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 31780_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51284_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 51284_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:24:41.60 -04:51:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165168_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 165168_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:08:07.15 -01:34:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 2.439 4262209687856533504 287.03040122278 -01.58107416080 11.6735 10.4032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77479_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 77479_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:14:58.06 -02:49:59.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83983_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 83983_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:42:23.59 -02:22:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.672 4259478810209044096 280.59846342863 -02.36754281735 11.9726 10.1219 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84001_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 84001_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:58:41.80 -02:20:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28067_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 28067_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65381_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 65381_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:13:47.78 -03:49:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100368_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 100368_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
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Considering the candidate 84634_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 84634_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
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Considering the candidate 146304_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 146304_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:53:14.18 +02:15:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39602_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 39602_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
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Considering the candidate 75227_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 75227_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
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Considering the candidate 124140_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 124140_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:24:46.96 +00:36:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73428_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 73428_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:10:44.92 -03:11:48.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 147949_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 147949_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
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Considering the candidate 31955_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
Preparing report for the candidate 31955_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
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Considering the candidate 70335_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 70335_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 18:43:24.30 -03:30:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.598 4258498011459868416 280.85158746594 -03.50376148596 11.6139 9.8855 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151452_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 151452_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks
**** FOUND 19:13:38.94 +01:20:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135709_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328
The candidate 135709_fd_Aql-03-Q2b1x1_2026-03-29_03-56-32_20.00sec_-15.00C_LIGHT_0328 did not pass the final checks