This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 11.22 11:35:42.27 -06:44:16.0
271.76494 51.49226 galactic Crt Second-epoch detections are separated by 0.7" and 5.5 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 | Gaia DR3 3593385595085122176 | 11:35:41.85 -06:44:16.7 (Gaia DR3) | T | P | 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
Gaia DR3 3593385595085122176,2461093.7687,11.22,0.05,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 3593385595085122176 20260222.2687 11.22CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:42.27 -06:44:16.0 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 07 35.41 -01 57 05.6 11.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7687,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2687 11.31CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:07:35.41 -01:57:05.6 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.55 11:35:21.85 -05:15:26.4
270.50635 52.75795 galactic Leo Second-epoch detections are separated by 1.3" and 5.3 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 | Gaia DR3 3593828384738056960 | 11:35:21.35 -05:15:27.2 (Gaia DR3) | T | P | 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!
TCP 2026 02 22.2687* 11 35 21.85 -05 15 26.4 13.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593828384738056960,2461093.7687,13.55,0.05,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 3593828384738056960 20260222.2687 13.55CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:21.85 -05:15:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 11.61 11:34:26.60 -05:45:07.7
270.56528 52.21384 galactic Leo Second-epoch detections are separated by 1.3" and 5.3 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 | Gaia DR3 3593704590896188416 | 11:34:26.15 -05:45:08.2 (Gaia DR3) | T | P | 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!
TCP 2026 02 22.2687* 11 34 26.60 -05 45 07.7 11.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593704590896188416,2461093.7687,11.61,0.05,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 3593704590896188416 20260222.2687 11.61CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:26.60 -05:45:07.7 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 11.45 11:35:09.35 -05:56:59.3
270.97281 52.12442 galactic Leo Second-epoch detections are separated by 0.7" and 5.5 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 | Gaia DR3 3593649993272219520 | 11:35:08.95 -05:56:58.4 (Gaia DR3) | T | P | 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!
TCP 2026 02 22.2687* 11 35 09.35 -05 56 59.3 11.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593649993272219520,2461093.7687,11.45,0.05,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 3593649993272219520 20260222.2687 11.45CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:09.35 -05:56:59.3 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 11.48 11:38:39.28 -03:51:39.9
270.59484 54.37633 galactic Vir Second-epoch detections are separated by 1.6" and 5.3 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 | Gaia DR3 3792149225480817152 | 11:38:38.85 -03:51:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5)
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!
TCP 2026 02 22.2687* 11 38 39.28 -03 51 39.9 11.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3792149225480817152,2461093.7687,11.48,0.05,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 3792149225480817152 20260222.2687 11.48CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:39.28 -03:51:39.9 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 36 57.37 -06 06 15.7 12.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593447511333914112,2461093.7687,12.08,0.05,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 3593447511333914112 20260222.2687 12.08CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:57.37 -06:06:15.7 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 12.57 11:34:53.45 -06:42:47.7
271.45972 51.41986 galactic Crt Second-epoch detections are separated by 0.3" and 5.4 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 | Gaia DR3 3593023031125810432 | 11:34:52.88 -06:42:48.1 (Gaia DR3) | T | P | 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
Gaia DR3 3593023031125810432,2461093.7687,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3593023031125810432 20260222.2687 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:53.45 -06:42:47.7 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 34 35.98 -01 22 40.4 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7687,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2687 12.60CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:35.98 -01:22:40.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 12.76 11:35:47.37 -06:38:17.5
271.72070 51.59026 galactic Leo Second-epoch detections are separated by 1.7" and 5.7 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 | Gaia DR3 3593399751296432512 | 11:35:46.86 -06:38:16.1 (Gaia DR3) | T | P | 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!
TCP 2026 02 22.2687* 11 35 47.37 -06 38 17.5 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593399751296432512,2461093.7687,12.76,0.05,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
Gaia DR3 3593399751296432512 20260222.2687 12.76CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:47.37 -06:38:17.5 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 10 41 57.68 -02 04 03.1 12.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7687,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2687 12.69CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:41:57.68 -02:04:03.1 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 11 02.63 -01 34 40.5 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7687,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2687 12.74CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:11:02.63 -01:34:40.5 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 12.77 11:30:07.58 -07:07:57.5
270.12739 50.48726 galactic Crt Second-epoch detections are separated by 1.0" and 5.6 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 | Gaia DR3 3593085119173128064 | 11:30:07.12 -07:07:58.1 (Gaia DR3) | T | P | 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
Gaia DR3 3593085119173128064,2461093.7687,12.77,0.05,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 3593085119173128064 20260222.2687 12.77CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:30:07.58 -07:07:57.5 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 12.97 11:37:07.02 -05:06:09.2
271.02099 53.10173 galactic Leo Second-epoch detections are separated by 0.8" and 5.4 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 | Gaia DR3 3593857594811070464 | 11:37:06.47 -05:06:09.9 (Gaia DR3) | T | P | 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!
TCP 2026 02 22.2687* 11 37 07.02 -05 06 09.2 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593857594811070464,2461093.7687,12.97,0.05,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 3593857594811070464 20260222.2687 12.97CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:07.02 -05:06:09.2 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.13 11:36:21.98 -06:22:34.5
271.72932 51.88878 galactic Leo Second-epoch detections are separated by 0.6" and 5.6 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 | Gaia DR3 3593410535959655296 | 11:36:21.52 -06:22:33.5 (Gaia DR3) | T | P | 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!
TCP 2026 02 22.2687* 11 36 21.98 -06 22 34.5 13.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593410535959655296,2461093.7687,13.13,0.05,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 3593410535959655296 20260222.2687 13.13CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:21.98 -06:22:34.5 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.17 11:35:33.58 -06:23:51.4
271.45843 51.77654 galactic Leo Second-epoch detections are separated by 1.4" and 5.4 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 | ATO J173.8878-06.3975 | 11:35:33.09 -06:23:51.0 (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!
TCP 2026 02 22.2687* 11 35 33.58 -06 23 51.4 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J173.8878-06.3975,2461093.7687,13.17,0.05,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 J173.8878-06.3975 20260222.2687 13.17CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:33.58 -06:23:51.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.16 11:37:32.95 -06:05:59.9
271.94557 52.26967 galactic Vir Second-epoch detections are separated by 2.8" and 5.6 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 J174.3856-06.0994 | 11:37:32.57 -06:05:58.0 (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!
TCP 2026 02 22.2687* 11 37 32.95 -06 05 59.9 13.2 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J174.3856-06.0994,2461093.7687,13.16,0.05,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 J174.3856-06.0994 20260222.2687 13.16CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:32.95 -06:05:59.9 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 09 14.51 -04 27 50.8 13.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7687,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2687 13.27CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:09:14.51 -04:27:50.8 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.23 11:23:28.23 -03:23:03.2
264.70625 52.83257 galactic Leo Second-epoch detections are separated by 0.1" and 5.4 pix This object is listed in comets.txt 4.3" 17.4mag 29P/Schwassmann-Wachmann 1
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.4.3" 17.4mag 29P/Schwassmann-Wachmann 1
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!
TCP 2026 02 22.2687* 11 23 28.23 -03 23 03.2 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7687,13.23,0.05,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
VARIABLE_NAME 20260222.2687 13.23CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:23:28.23 -03:23:03.2 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.38 11:38:12.91 -04:52:15.2
271.24209 53.43487 galactic Vir Second-epoch detections are separated by 0.4" and 5.4 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 | ATO J174.5521-04.8707 | 11:38:12.52 -04:52:14.7 (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!
TCP 2026 02 22.2687* 11 38 12.91 -04 52 15.2 13.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J174.5521-04.8707,2461093.7687,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J174.5521-04.8707 20260222.2687 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:12.91 -04:52:15.2 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 37 12.39 -06 38 16.8 13.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593390950908435584,2461093.7687,13.31,0.05,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 3593390950908435584 20260222.2687 13.31CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:12.39 -06:38:16.8 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.40 11:36:35.90 -06:54:18.8
272.20492 51.44593 galactic Crt Second-epoch detections are separated by 3.4" and 5.7 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 | Gaia DR3 3593332161396442880 | 11:36:35.50 -06:54:17.4 (Gaia DR3) | T | P | 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
Gaia DR3 3593332161396442880,2461093.7687,13.40,0.05,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 3593332161396442880 20260222.2687 13.40CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:35.90 -06:54:18.8 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.53 11:35:37.50 -07:02:21.4
271.96028 51.21583 galactic Crt Second-epoch detections are separated by 5.1" and 5.4 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 | Gaia DR3 3592954552167278592 | 11:35:37.06 -07:02:19.3 (Gaia DR3) | T | P | 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
Gaia DR3 3592954552167278592,2461093.7687,13.53,0.05,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 3592954552167278592 20260222.2687 13.53CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:37.50 -07:02:21.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.61 11:34:36.71 -07:02:11.8
271.60322 51.10159 galactic Crt Second-epoch detections are separated by 0.5" and 5.6 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 | Gaia DR3 3592997982876571904 | 11:34:36.25 -07:02:10.7 (Gaia DR3) | T | P | 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
Gaia DR3 3592997982876571904,2461093.7687,13.61,0.05,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 3592997982876571904 20260222.2687 13.61CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:36.71 -07:02:11.8 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.63 11:35:45.71 -06:20:28.0
271.48754 51.84996 galactic Leo Second-epoch detections are separated by 1.8" and 5.4 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 | Gaia DR3 3593602027077221632 | 11:35:45.22 -06:20:27.0 (Gaia DR3) | T | P | 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!
TCP 2026 02 22.2687* 11 35 45.71 -06 20 28.0 13.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593602027077221632,2461093.7687,13.63,0.05,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 3593602027077221632 20260222.2687 13.63CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:45.71 -06:20:28.0 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 36 02.03 -05 40 52.8 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J113601.58-054053.3,2461093.7687,13.50,0.05,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 J113601.58-054053.3 20260222.2687 13.50CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:02.03 -05:40:52.8 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.59 11:35:58.57 -07:02:14.8
272.08245 51.25760 galactic Crt Second-epoch detections are separated by 6.5" and 5.6 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 | Gaia DR3 3592953998116128000 | 11:35:58.47 -07:02:24.4 (Gaia DR3) | T | P | 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
Gaia DR3 3592953998116128000,2461093.7687,13.59,0.05,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 3592953998116128000 20260222.2687 13.59CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:58.57 -07:02:14.8 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 35 49.90 -06 25 45.2 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0346 Leo,2461093.7687,13.54,0.05,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
V0346 Leo 20260222.2687 13.54CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:49.90 -06:25:45.2 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.82 11:36:12.54 -05:57:15.7
271.35305 52.24377 galactic Leo Second-epoch detections are separated by 0.5" and 5.6 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 J174.0502-05.9545 | 11:36:12.06 -05:57:16.2 (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!
TCP 2026 02 22.2687* 11 36 12.54 -05 57 15.7 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J174.0502-05.9545,2461093.7687,13.82,0.05,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 J174.0502-05.9545 20260222.2687 13.82CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:12.54 -05:57:15.7 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.80 11:34:09.21 -06:32:15.3
271.06781 51.48875 galactic Leo Second-epoch detections are separated by 0.5" and 5.6 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 | Gaia DR3 3593219946786574976 | 11:34:08.74 -06:32:14.6 (Gaia DR3) | T | P | 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!
TCP 2026 02 22.2687* 11 34 09.21 -06 32 15.3 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593219946786574976,2461093.7687,13.80,0.05,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 3593219946786574976 20260222.2687 13.80CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:09.21 -06:32:15.3 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.72 11:34:17.70 -06:19:59.7
270.96192 51.68537 galactic Leo Second-epoch detections are separated by 3.3" and 5.6 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 | Gaia DR3 3593610891889686528 | 11:34:17.20 -06:20:00.3 (Gaia DR3) | T | P | 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!
TCP 2026 02 22.2687* 11 34 17.70 -06 19 59.7 13.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593610891889686528,2461093.7687,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3593610891889686528 20260222.2687 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:17.70 -06:19:59.7 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.98 11:35:31.86 -05:34:43.2
270.81913 52.49540 galactic Leo Second-epoch detections are separated by 2.1" and 5.6 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 J173.8810-05.5784 | 11:35:31.86 -05:34:43.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
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!
TCP 2026 02 22.2687* 11 35 31.86 -05 34 43.2 14.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J173.8810-05.5784,2461093.7687,13.98,0.05,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 J173.8810-05.5784 20260222.2687 13.98CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:31.86 -05:34:43.2 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.89 11:36:40.28 -05:43:54.0
271.34854 52.49439 galactic Leo Second-epoch detections are separated by 1.1" and 5.6 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 | Gaia DR3 3593750907823419520 | 11:36:39.68 -05:43:53.1 (Gaia DR3) | T | P | 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!
TCP 2026 02 22.2687* 11 36 40.28 -05 43 54.0 13.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3593750907823419520,2461093.7687,13.89,0.05,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
Gaia DR3 3593750907823419520 20260222.2687 13.89CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:40.28 -05:43:54.0 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.96 11:37:59.28 -06:08:18.2
272.13277 52.28569 galactic Vir Second-epoch detections are separated by 5.4" and 5.7 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 J174.4951-06.1383 | 11:37:59.28 -06:08:18.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
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!
TCP 2026 02 22.2687* 11 37 59.28 -06 08 18.2 14.0 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J174.4951-06.1383,2461093.7687,13.96,0.05,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 J174.4951-06.1383 20260222.2687 13.96CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:59.28 -06:08:18.2 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 13.94 11:35:08.45 -07:06:28.6
271.84107 51.09941 galactic Crt Second-epoch detections are separated by 4.5" and 6.2 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 | Gaia DR3 3592948092536460800 | 11:35:07.94 -07:06:29.6 (Gaia DR3) | T | P | 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
Gaia DR3 3592948092536460800,2461093.7687,13.94,0.05,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
Gaia DR3 3592948092536460800 20260222.2687 13.94CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:08.45 -07:06:28.6 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 33 22.99 -06 41 22.5 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7687,14.08,0.05,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
target 20260222.2687 14.08CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:33:22.99 -06:41:22.5 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 14.05 11:35:49.30 -05:42:12.3
271.02068 52.41984 galactic Leo Second-epoch detections are separated by 1.1" and 5.6 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 J173.9535-05.7035 | 11:35:49.30 -05:42:12.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
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!
TCP 2026 02 22.2687* 11 35 49.30 -05 42 12.3 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J173.9535-05.7035,2461093.7687,14.05,0.05,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 J173.9535-05.7035 20260222.2687 14.05CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:49.30 -05:42:12.3 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_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
target,2461093.7687,13.96,0.05,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
target 20260222.2687 13.96CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:01.84 -06:53:25.7 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 36 08.91 -06 26 00.4 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7687,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2687 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:08.91 -06:26:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 36 41.49 -06 25 11.2 14.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7687,14.01,0.05,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
target 20260222.2687 14.01CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:41.49 -06:25:11.2 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_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
target,2461093.7687,14.11,0.05,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
target 20260222.2687 14.11CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:21.37 -07:05:27.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2687 2461093.7687 14.23 11:38:21.06 -04:05:24.8
270.66788 54.13880 galactic Vir Second-epoch detections are separated by 1.5" and 5.7 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 | target | 11:38:21.06 -04:05:24.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
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!
TCP 2026 02 22.2687* 11 38 21.06 -04 05 24.8 14.2 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7687,14.23,0.05,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
target 20260222.2687 14.23CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:21.06 -04:05:24.8 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 37 19.12 -06 23 29.6 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7687,14.36,0.05,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
target 20260222.2687 14.36CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:19.12 -06:23:29.6 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 23 33.96 -06 19 03.8 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7687,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2687 14.36CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:23:33.96 -06:19:03.8 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 10 45 24.33 -02 31 15.1 14.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7687,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2687 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:45:24.33 -02:31:15.1 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2687* 11 37 39.25 -04 55 24.7 14.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7687,14.36,0.05,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
target 20260222.2687 14.36CV 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:39.25 -04:55:24.7 ;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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20_00sec_-14_90C_LIGHT_0224_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: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461093.76895617 22.02.2026 06:27:07.813 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 43
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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: 11 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): 6833
Objects passed selection criteria: 6828
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 6304
Average stars matched: 6047.75 (95.9351 %)
Memory usage VmPeak: 112604 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 02:51:56 CST 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: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461093.76895617 22.02.2026 06:27:07.813 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 280
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
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: 51 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): 35060
Objects passed selection criteria: 35003
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 33311.5
Average stars matched: 31416 (94.3098 %)
Memory usage VmPeak: 136232 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 02:55:29 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE=
FRAME_EDGE_OFFSET_PIX= 100
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Leo-08-Q2b1x1
#######################################
########### Starting Leo-08-Q2b1x1 ###########
Processing Leo-08-Q2b1x1
server tau has sufficient free disk space available: 1054529 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1054529 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.png' -> 'transient_report/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits_preview.png'
Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
renamed 'Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.png' -> 'transient_report/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits_preview.png'
Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 691.9982
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 502.2529
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1254.6674
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 549.3174
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1252.8452
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 549.3449
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.81311
INFO: SECOND_EPOCH__SD_ratio= 0.000
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
No bad regions file found ../bad_region.lst
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.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: 2461093.76839170
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
Saving wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits to local_wcs_cache/
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
Saving wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits to local_wcs_cache/
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits exists and is non-empty
Saving wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits to local_wcs_cache/
'wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits' -> 'local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits'
wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.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 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:35.286 -01:59:58.19
Angular distance between the image centers 0.00 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 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:36.198 -01:59:29.03
Angular distance between the image centers 0.01 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 11:08:35.286 -01:59:58.19
Second-epoch second image center 11:08:36.198 -01:59:29.03
Angular distance between the image centers 0.00895 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.XMASEn4BKB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.yGFvRP7yKJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits &> /tmp/tmp.1U8gVaLP5d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.g7j7pSdGM9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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 3372 out of 6399 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.879752
a=0.000000 b=1.000000 c=22.879752
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 39 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.4 pix Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
2.4 pix Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
Limiting magnitude estimates:
15.2 mag. Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.2 mag. Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
15.1 mag. Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
15.1 mag. Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.XMASEn4BKB (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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=432, passed=6399
Got 6399 stars (including 5960 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 6399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 947 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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.yGFvRP7yKJ (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/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=407, passed=6519
Got 6519 stars (including 6107 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 6519 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.29"
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_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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.1U8gVaLP5d (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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=587, passed=6268
Got 6268 stars (including 5677 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat
util/solve_plate_with_UCAC5 got 6268 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 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: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits -region wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.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.g7j7pSdGM9 (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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=573, passed=6254
Got 6254 stars (including 5678 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 6254 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 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: 0.41"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Leo-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20430.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 24s
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: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20424_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 20424_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20430_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 20430_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20468_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20468_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:00:24.15 -02:42:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 1.100 3801762663667379968 165.10089962507 -02.70733738931 12.1730 11.8880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20483_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20483_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:57.10 -06:06:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 5.526 3593447511332803200 174.23643325910 -06.10376989061 10.6485 10.0896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20494_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20494_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:02:02.12 -02:30:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.510 3801783210786956032 165.50895322017 -02.50568660115 12.1713 11.6816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20499_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20499_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:16:16.53 -03:29:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.577 3790018127132099584 169.06880574801 -03.48972789056 12.3821 11.8969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20502_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20502_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:09:02.78 -05:01:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.679 3788217676841690112 167.26169121059 -05.02128957487 12.1895 11.7683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20506_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20506_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:04:48.97 -02:53:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 1.182 3789704422720870272 166.20423642301 -02.88906880107 12.2974 11.7334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20512_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20512_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:06:59.13 -03:27:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.688 3789464866624903168 166.74646022670 -03.46107898603 12.2876 11.7310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20516_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20516_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:10:25.08 -01:55:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.284 3791368430490486272 167.60453325745 -01.93151164796 12.2959 11.5832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20518_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20518_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:01:40.67 -04:05:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.973 3789312378106826240 165.41972872921 -04.09062353103 12.1761 11.4975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20525_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20525_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:03:06.58 -02:34:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.627 3789769951037564672 165.77748562014 -02.57742330449 12.3413 11.7766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20528_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20528_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:07:10.59 -02:07:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.689 3791302837750347136 166.79430138463 -02.11990760320 12.4285 11.9376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20530_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20530_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:07:48.29 -03:52:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.840 3789368835451997568 166.95137665468 -03.86730071868 12.4032 11.9427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20531_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20531_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:07:11.79 -01:46:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.366 3791421829819490560 166.79921555768 -01.77423145928 12.4655 11.9850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20532_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20532_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:06:37.74 -01:47:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.302 3791421005185768448 166.65733154322 -01.78853565027 12.2625 11.4899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20535_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20535_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:03:11.36 -02:52:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.806 3789725931917889152 165.79745976884 -02.87800965022 12.4505 11.9814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20538_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20538_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:10:49.42 -03:24:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.253 3790164121664522112 167.70593078251 -03.40537430867 12.4306 11.9314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20539_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20539_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:10:52.09 -02:35:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.834 3791117883573780480 167.71691999130 -02.59194166462 12.4822 12.0117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20540_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20540_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:06:58.43 -03:23:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.016 3789466481532605184 166.74346145600 -03.39513575673 12.3001 11.5951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20541_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20541_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:05:26.91 -00:13:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.694 3804205400543205632 166.36231332743 -00.22956889191 12.3851 11.9220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20542_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20542_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:01:11.37 -02:01:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.735 3801874401532577536 165.29753641899 -02.02398608486 12.3928 11.8464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20544_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20544_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:06:58.66 -02:17:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.285 3791294350894972672 166.74434315158 -02.28880701090 12.4743 11.9194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20546_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20546_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:01:31.74 -04:34:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.247 3788908651180380800 165.38225876876 -04.57984872723 12.3376 11.8235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20547_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20547_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 10:58:24.23 -02:43:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.703 3801720160667096960 164.60112681853 -02.71873771961 12.3847 11.9420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20548_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20548_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:01:38.48 -03:16:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.355 3789618562030780288 165.41039578214 -03.28274319992 12.3811 11.8783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20549_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20549_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:12:07.60 -00:50:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.734 3791881837996908160 168.03185538841 -00.83463285290 12.4203 11.9843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20550_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20550_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:07:23.50 -02:53:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.824 3791001335341172480 166.84793179196 -02.88316045615 12.3696 11.8089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20551_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20551_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:02:15.93 -03:47:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.642 3789534135857484032 165.56653809323 -03.79648239136 12.2761 11.5994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20553_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20553_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:14:21.97 -02:43:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.686 3790326230906045568 168.59173240604 -02.72958717387 12.2749 11.5773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20554_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20554_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:10:25.42 -02:23:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.708 3791136399177469568 167.60581141907 -02.39238827421 12.4963 11.9029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20557_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20557_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:13:44.43 -03:54:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.088 3789907798012286080 168.43542339814 -03.90692062676 11.9524 10.9359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20558_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20558_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:04:34.30 -02:12:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.039 3803298818846621056 166.14319257742 -02.20891421201 12.8577 12.3553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20559_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20559_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:12:00.89 -03:15:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.352 3790186975182294656 168.00376277314 -03.26480761475 12.4266 11.8481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20560_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20560_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:10:04.33 -03:01:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.490 3790959515243909504 167.51844166493 -03.03191962314 12.2866 11.5087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20561_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20561_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:10:28.40 -03:04:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.101 3790946668997542528 167.61833733363 -03.08288895142 12.5092 12.0007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20563_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20563_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:12:39.83 -01:29:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.808 3791763537417788288 168.16618213894 -01.48348089790 12.4467 11.8741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20564_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20564_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:06:06.55 -05:12:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.848 3788378038036382208 166.52748906075 -05.20317596481 12.3982 11.9838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20566_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 20566_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:09:37.50 -00:50:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.509 3803868060927628672 167.40638204291 -00.84913427545 12.5315 12.0816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 31s
Prepared the HTML report for the field Leo-08-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 ####
11:35:42.27 -06:44:16.0
11:07:35.41 -01:57:05.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Creating symlink local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Creating symlink local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
Creating symlink local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits exists and is non-empty
wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.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 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:35.286 -01:59:58.19
Angular distance between the image centers 0.00 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 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:36.198 -01:59:29.03
Angular distance between the image centers 0.01 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 11:08:35.286 -01:59:58.19
Second-epoch second image center 11:08:36.198 -01:59:29.03
Angular distance between the image centers 0.00895 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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.uraIheiQpP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.pUhIzlRQr3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits &> /tmp/tmp.A87I2gPB0T
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.zGkdKij1o9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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 3398 out of 34371 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.774901
a=0.000000 b=1.000000 c=22.774901
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 155 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.3 pix Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
2.3 pix Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
Limiting magnitude estimates:
15.3 mag. Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.3 mag. Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
15.3 mag. Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
15.3 mag. Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.uraIheiQpP (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/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1404, passed=34365
Got 34365 stars (including 32904 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 34365 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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: 0.31"
Estimated accuracy of the plate solution: 0.28"
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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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.pUhIzlRQr3 (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/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1420, passed=33111
Got 33111 stars (including 31640 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 33111 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.30"
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_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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.A87I2gPB0T (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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=2039, passed=33513
Got 33513 stars (including 31443 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat
util/solve_plate_with_UCAC5 got 33513 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 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: 0.40"
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 961 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: 0.39"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits -region wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-26-19_20.00sec_-14.90C_LIGHT_0224.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.zGkdKij1o9 (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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.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_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2037, passed=33489
Got 33489 stars (including 31412 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 33489 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-08-Q2b1x1_002749_TTUQ2b1x1_19475_jzUtZzfi/Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Leo-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52956.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52187.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out53026.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out51793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53105.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 107s
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: 35s
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Considering the candidate 51748_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51748_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:45.10 -04:05:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 0.389 3792118370435723648 174.18791389665 -04.08683025065 13.3304 12.5605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51753_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51753_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 51755_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51755_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 51757_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51757_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:40.41 -02:28:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.942 3792592294307138048 174.41842716230 -02.47610210216 13.3052 12.6877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51758_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51758_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:06.81 -05:24:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 4.265 3785885788773866368 173.52931801696 -05.40027748332 13.2989 12.7443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51759_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51759_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:16:57.88 +02:24:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.521 3810974342016920448 169.24158730904 +02.41529115786 14.4066 13.7706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51761_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51761_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:31:24.70 -06:26:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.759 3593280007609080320 172.85242532652 -06.43760413333 13.2580 12.7688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51765_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51765_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:38:02.44 -04:54:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 4.507 3593866975019652480 174.50898830336 -04.90439888667 13.0409 12.5110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51766_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51766_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 51767_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51767_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:30:43.17 -06:25:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 5.278 3593269115572015488 172.68134836451 -06.42241125433 13.2398 12.5750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51772_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51772_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:17:59.74 -04:19:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.354 3786818518231860352 169.49868623115 -04.32560331050 14.5583 13.9139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51774_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51774_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:25:49.40 +01:41:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 0.400 3798678366044637440 171.45579172260 +01.68739703403 14.2860 13.7609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51776_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51776_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 10:40:05.32 +03:01:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.517 3857418640886857984 160.02252815215 +03.02456046870 13.5004 12.9687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51777_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51777_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 51778_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51778_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:30:00.58 -06:37:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.178 3593257776858326912 172.50180751305 -06.63300113886 12.9355 12.3091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51779_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51779_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 10:50:02.03 +03:06:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.832 3809766425414779648 162.50868806350 +03.10224977939 13.7292 13.1734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51780_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51780_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:31:18.32 -06:36:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 5.078 3593249805399108736 172.82771560136 -06.61346234987 12.9437 12.3363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51781_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51781_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:02:25.92 +00:05:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.328 3804619886362795008 165.60807067023 +00.09772426925 14.1256 13.5023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51782_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51782_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51783_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51783_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:39:36.60 -01:03:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 3.593 3793948400165144192 174.90150190571 -01.05539920758 12.7364 12.1214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51785_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51785_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:13:27.17 +00:25:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.242 3810120639957521792 168.36353789729 +00.42920333027 14.0038 13.4833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51786_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51786_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 51787_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51787_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 51789_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51789_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 10:43:30.11 -03:20:31.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)
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Considering the candidate 51792_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51792_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:30:56.95 -07:08:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.934 3593078281585234304 172.73766240157 -07.13769689596 12.2269 11.7340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51793_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 51793_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 51794_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51794_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 10:56:42.98 +02:17:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.108 3808680211005261056 164.17965850001 +02.29666780643 13.6149 13.1017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51798_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51798_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:29:46.10 -07:06:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 4.008 3593087971031411712 172.44319744737 -07.10932619071 11.2720 10.7406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51799_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 51799_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 51806_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51806_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:33:37.93 -06:32:12.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 51819_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51819_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:35:14.26 -06:29:32.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 51840_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51840_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:22.57 -06:15:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 5.354 3593435897742130688 174.34261118540 -06.26225907468 9.7968 9.4648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51863_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51863_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:07:35.42 -01:57:05.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51864_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51864_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:35:42.34 -06:44:16.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51870_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51870_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:35:35.39 -06:55:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 3.931 3593002758880211328 173.89647373264 -06.92695771599 10.2194 9.8714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51872_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 51872_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 51876_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 51876_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 51931_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51931_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:20.76 -07:05:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 4.297 3592997295681760256 173.58536949879 -07.09603708168 10.6939 10.3097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51940_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51940_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:38:26.59 -04:55:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 3.758 3599859553909328000 174.60974798168 -04.93226760942 10.4272 9.7594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51944_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51944_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:19.59 -05:24:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 4.851 3593813683065428608 174.33027192127 -05.40700307753 10.5966 9.9385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51954_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 51954_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 51975_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51975_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:33.16 -05:38:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 5.100 3593755649467315968 174.13677315180 -05.63721117931 11.1238 10.7589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51988_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51988_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:54.39 -05:48:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 5.836 3593737748043655296 174.22499559978 -05.81204809987 10.8656 10.2330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51998_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 51998_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52006_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52006_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 10:51:57.80 -04:08:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.824 3801124397163781504 162.99088356325 -04.13538991926 12.4062 11.8350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52026_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52026_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:47.55 -05:51:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 2.371 3593734346429584640 174.44752544060 -05.85547069910 11.2830 10.7878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52067_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52067_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52081_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52081_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52089_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52089_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:57.35 -03:28:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.129 3792455439469265280 174.48754114760 -03.47705762062 11.2577 10.6380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52090_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52090_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:33:58.04 -06:22:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.957 3593609105183289088 173.49102641668 -06.37521053430 11.4526 10.9730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52098_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52098_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52100_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52100_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:37.98 -05:29:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 2.997 3593764922301001344 174.40745650545 -05.49045945091 11.7574 11.5245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52104_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52104_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52106_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52106_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:33.79 -06:31:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.224 3593396487122214784 174.14025771555 -06.52054439116 11.5439 11.1151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52110_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52110_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:02.90 -06:23:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.104 3593421432292274304 174.26098837169 -06.39838209863 11.6004 11.1842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52111_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52111_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52112_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52112_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:37.97 -07:04:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.490 3592994821780640128 173.65755775065 -07.07530718792 11.6796 11.2974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52118_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52118_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52119_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52119_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:28.42 -06:40:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.028 3593027051215199360 173.61730825411 -06.67429992354 11.5446 10.9953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52123_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52123_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52150_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52150_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:33.65 -06:20:23.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
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Considering the candidate 52155_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52155_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52163_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52163_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:39.71 -05:00:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 3.274 3593864569837172608 174.41455360954 -05.00576706299 11.7623 11.3240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52183_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52183_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:35:56.06 -05:00:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.220 3786015664288839040 173.98268624307 -05.00582250051 11.8057 11.1650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52187_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52187_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:16.14 -06:22:49.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
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Considering the candidate 52199_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52199_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:38:02.07 -04:59:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.991 3593854227556715392 174.50725771345 -04.99876913630 11.8859 11.4400 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52237_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52237_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52256_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52256_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:31.93 -06:48:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.599 3593335223708697344 174.13158634979 -06.79948090816 11.8436 11.4013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52265_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52265_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:40.51 -05:56:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 2.466 3593732319205020160 174.41813256741 -05.93757888215 12.0645 11.6600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52271_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52271_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:57.65 -04:42:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.755 3786030404616592640 174.23860704947 -04.71598787965 12.0303 11.5458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52273_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52273_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52274_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52274_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:32:46.51 -06:54:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.225 3593180158209531264 173.19354862300 -06.91620447781 11.5368 10.8686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52281_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52281_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52303_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52303_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52310_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52310_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52312_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52312_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 52314_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52314_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:04.18 -06:40:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.643 3593213246637589504 173.51677779064 -06.67435299506 11.8331 11.1839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52339_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52339_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52343_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52343_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:51.81 -05:45:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.614 3593750250693102976 174.21519330169 -05.75810155058 12.0860 11.5522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52352_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52352_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52356_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52356_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52365_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52365_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:24:33.38 +00:11:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.733 3797868983752234240 171.13901921219 +00.19869574772 13.4468 12.9554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52368_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52368_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52377_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52377_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:38.28 -06:51:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.561 3593332612367715072 174.15828668794 -06.85219079420 12.1374 11.6550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52389_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52389_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:32:21.24 -07:02:18.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)
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Considering the candidate 52411_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52411_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:42.09 -06:36:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.558 3593367831100445952 174.42479841268 -06.60810735909 12.2455 11.8869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52418_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52418_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:29:07.38 -02:53:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.899 3793439949052559744 172.28096919926 -02.89646337850 13.1937 12.5723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52419_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52419_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52420_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52420_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:41.61 -06:31:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.702 3593415689920057728 174.42246569649 -06.52142515175 12.0689 11.5695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52423_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52423_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:27.82 -04:50:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.955 3786027591413976192 174.11453696717 -04.83534876949 12.2581 11.7722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52435_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52435_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52437_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52437_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:39:05.45 -02:53:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.642 3792515633435490944 174.77156102247 -02.89706327955 12.1717 11.4979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52451_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52451_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52452_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52452_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52453_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52453_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:05:57.99 -05:23:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.221 3787997052961638144 166.49162760626 -05.39367237617 13.6527 13.2490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52472_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52472_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:01.51 -06:00:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 5.875 3593637585110591360 174.25486880339 -06.00679829772 12.7596 12.4353 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52477_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52477_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52481_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52481_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:38.36 -06:40:37.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
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Considering the candidate 52527_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52527_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:38:37.62 -02:56:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.365 3792509964078661376 174.65531757702 -02.93744555111 12.2471 11.6238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52538_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52538_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:35:17.72 -06:37:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 5.160 3593399506483641728 173.82239938408 -06.61881199179 12.4347 11.8517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52553_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52553_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:30:56.86 -06:58:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 4.279 3593187575617035520 172.73574801340 -06.97924038627 12.6504 12.1476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52559_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52559_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52560_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52560_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:19.86 -06:40:20.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 52565_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52565_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52568_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52568_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:33:50.31 -06:59:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.792 3593010833418678400 173.45925951302 -06.99053545632 12.4210 11.7360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52573_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52573_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:14:03.08 +02:50:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.800 3811807565672291712 168.51325541437 +02.83667580096 13.8477 13.3012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52576_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52576_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:35:41.00 -07:02:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.993 3592953796253069184 173.92055884422 -07.04343244372 12.4655 11.9527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52587_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52587_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:38:04.70 -06:12:26.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
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Considering the candidate 52600_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52600_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52622_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52622_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:39.50 -06:41:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 5.645 3593026187926433920 173.66300982766 -06.69287031168 12.4694 11.9389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52655_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52655_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52656_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52656_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:31:37.81 -00:49:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 2.165 3797125237150765056 172.90699954938 -00.82095482218 13.8965 13.3322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52658_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52658_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52659_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52659_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52662_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52662_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:56.24 -06:38:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.090 3593026879416509952 173.73350432781 -06.63910359038 12.6804 12.2426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52696_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52696_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52707_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52707_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52721_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52721_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:36:49.98 -06:12:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 4.556 3593440188413865984 174.20699726600 -06.19994150905 12.5196 11.8542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52723_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52723_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52737_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52737_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52754_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52754_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:35:11.31 -05:59:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 3.034 3593648859400594816 173.79629113656 -05.98906646436 13.0544 12.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52764_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52764_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:03.24 -06:51:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 3.272 3593017121250816256 173.51273635434 -06.85761240858 12.6322 12.0434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52779_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52779_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52804_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52804_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52817_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52817_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:26:50.76 +01:39:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 0.365 3798675136229258368 171.71144753215 +01.66367023460 14.1818 13.6700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52818_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52818_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:53.87 -06:27:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 5.573 3593594360559730432 173.72294591490 -06.45401709458 12.9001 12.3333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52824_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52824_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:33:10.87 -06:49:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 3.296 3593205236522915968 173.29438348420 -06.81753652581 12.9501 12.5281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52831_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52831_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52835_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52835_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:06:03.43 -07:01:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.440 3784542323003766400 166.51412315658 -07.02608549356 14.0749 13.5543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52842_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52842_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
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Considering the candidate 52849_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52849_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:38:02.07 -05:28:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 4.328 3593785748598168192 174.50741755842 -05.47019708664 12.8700 12.2314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52851_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52851_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:26.74 -04:46:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 5.794 3792030959261328640 174.35981035809 -04.76699831746 12.9276 12.2555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52856_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52856_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:23:34.33 +00:27:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 4.268 3797936848530964224 170.89416690350 +00.46092927563 14.3974 13.8412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52893_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52893_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:54.27 -06:41:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 3.002 3593023477802409984 173.72528997254 -06.69247671950 13.1952 12.7496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52900_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52900_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:34:47.71 -06:57:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 2.915 3593000353698522624 173.69798798374 -06.95708320820 13.0199 12.5033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52902_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52902_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:03:20.59 -01:09:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 0.365 3803619468220370688 165.83588198480 -01.16414807945 14.7119 14.0043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52907_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52907_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:35:12.17 -06:22:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 5.612 3593600996285068288 173.79914290867 -06.37579374071 12.9353 12.3706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52941_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52941_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 52942_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52942_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:27.02 -04:06:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 3.816 3792137714968425856 174.36158671989 -04.11274335426 13.1014 12.5850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52956_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52956_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:12:56.73 -05:37:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 4.064 3785115409079835136 168.23723732717 -05.61721096192 14.6296 13.9472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52966_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 52966_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52980_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52980_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:35:48.83 -06:41:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 4.587 3593386179200675968 173.95217598167 -06.69002011537 13.1139 12.5834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52990_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52990_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:33:38.35 -06:47:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 4.351 3593206202891219328 173.40857468158 -06.78680285163 13.2467 12.7644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52993_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 52993_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:38:24.00 -05:07:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 3.064 3593847183810379136 174.59933972553 -05.12329320492 13.3292 12.8533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53014_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 53014_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:09:02.57 +00:06:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.395 3804279656233454976 167.26081808238 +00.10989068548 14.7775 14.2146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53026_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 53026_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:31:31.92 -02:18:33.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)
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Considering the candidate 53030_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 53030_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:51.26 -06:39:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 2.372 3593340308950012032 174.46348271748 -06.65809868174 13.2163 12.6860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53036_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 53036_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53062_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 53062_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:38:13.95 -03:43:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 3.005 3792259588960451968 174.55731287686 -03.72697829854 13.1342 12.4840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53086_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 53086_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53105_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
Preparing report for the candidate 53105_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53112_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 53112_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53193_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 53193_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
**** FOUND 11:37:49.95 -05:30:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 4.912 3593762074738431360 174.45677226121 -05.51344579800 13.2996 12.9304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04751_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 04751_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33674_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225
The candidate 33674_Leo-08-Q2b1x1_2026-02-22_00-27-07_20.00sec_-15.00C_LIGHT_0225 did not pass the final checks
Rejecting candidate due to large distance (31.8") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 149s
Prepared the HTML report for the field Leo-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:35:42.27 -06:44:16.0
11:07:35.41 -01:57:05.6
11:35:21.85 -05:15:26.4
11:34:26.60 -05:45:07.7
11:35:09.35 -05:56:59.3
11:38:39.28 -03:51:39.9
11:36:57.37 -06:06:15.7
11:34:53.45 -06:42:47.7
11:34:35.98 -01:22:40.4
11:35:47.37 -06:38:17.5
10:41:57.68 -02:04:03.1
11:11:02.63 -01:34:40.5
11:30:07.58 -07:07:57.5
11:37:07.02 -05:06:09.2
11:36:21.98 -06:22:34.5
11:35:33.58 -06:23:51.4
11:37:32.95 -06:05:59.9
11:09:14.51 -04:27:50.8
11:38:12.91 -04:52:15.2
11:37:12.39 -06:38:16.8
11:36:35.90 -06:54:18.8
11:35:37.50 -07:02:21.4
11:34:36.71 -07:02:11.8
11:35:45.71 -06:20:28.0
11:36:02.03 -05:40:52.8
11:35:58.57 -07:02:14.8
11:35:49.90 -06:25:45.2
11:36:12.54 -05:57:15.7
11:34:09.21 -06:32:15.3
11:34:17.70 -06:19:59.7
11:35:31.86 -05:34:43.2
11:36:40.28 -05:43:54.0
11:37:59.28 -06:08:18.2
11:35:08.45 -07:06:28.6
11:33:22.99 -06:41:22.5
11:35:49.30 -05:42:12.3
11:37:01.84 -06:53:25.7
11:36:08.91 -06:26:00.4
11:36:41.49 -06:25:11.2
11:35:21.37 -07:05:27.4
11:38:21.06 -04:05:24.8
11:37:19.12 -06:23:29.6
11:23:33.96 -06:19:03.8
10:45:24.33 -02:31:15.1
11:37:39.25 -04:55:24.7
########### Completed Leo-08-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
11:35:42.27 -06:44:16.0
11:07:35.41 -01:57:05.6
11:35:21.85 -05:15:26.4
11:34:26.60 -05:45:07.7
11:35:09.35 -05:56:59.3
11:38:39.28 -03:51:39.9
11:36:57.37 -06:06:15.7
11:34:53.45 -06:42:47.7
11:34:35.98 -01:22:40.4
11:35:47.37 -06:38:17.5
10:41:57.68 -02:04:03.1
11:11:02.63 -01:34:40.5
11:30:07.58 -07:07:57.5
11:37:07.02 -05:06:09.2
11:36:21.98 -06:22:34.5
11:35:33.58 -06:23:51.4
11:37:32.95 -06:05:59.9
11:09:14.51 -04:27:50.8
11:23:28.23 -03:23:03.2
11:38:12.91 -04:52:15.2
11:37:12.39 -06:38:16.8
11:36:35.90 -06:54:18.8
11:35:37.50 -07:02:21.4
11:34:36.71 -07:02:11.8
11:35:45.71 -06:20:28.0
11:36:02.03 -05:40:52.8
11:35:58.57 -07:02:14.8
11:35:49.90 -06:25:45.2
11:36:12.54 -05:57:15.7
11:34:09.21 -06:32:15.3
11:34:17.70 -06:19:59.7
11:35:31.86 -05:34:43.2
11:36:40.28 -05:43:54.0
11:37:59.28 -06:08:18.2
11:35:08.45 -07:06:28.6
11:33:22.99 -06:41:22.5
11:35:49.30 -05:42:12.3
11:37:01.84 -06:53:25.7
11:36:08.91 -06:26:00.4
11:36:41.49 -06:25:11.2
11:35:21.37 -07:05:27.4
11:38:21.06 -04:05:24.8
11:37:19.12 -06:23:29.6
11:23:33.96 -06:19:03.8
10:45:24.33 -02:31:15.1
11:37:39.25 -04:55:24.7
###################################################################################
11:35:42.27 -06:44:16.0 -- not an asteroid (will add it to exclusion list)
11:07:35.41 -01:57:05.6 -- asteroid (will NOT add it to exclusion list)
11:35:21.85 -05:15:26.4 -- not an asteroid (will add it to exclusion list)
11:34:26.60 -05:45:07.7 -- not an asteroid (will add it to exclusion list)
11:35:09.35 -05:56:59.3 -- not an asteroid (will add it to exclusion list)
11:38:39.28 -03:51:39.9 -- not an asteroid (will add it to exclusion list)
11:36:57.37 -06:06:15.7 -- not an asteroid (will add it to exclusion list)
11:34:53.45 -06:42:47.7 -- not an asteroid (will add it to exclusion list)
11:34:35.98 -01:22:40.4 -- asteroid (will NOT add it to exclusion list)
11:35:47.37 -06:38:17.5 -- not an asteroid (will add it to exclusion list)
10:41:57.68 -02:04:03.1 -- asteroid (will NOT add it to exclusion list)
11:11:02.63 -01:34:40.5 -- asteroid (will NOT add it to exclusion list)
11:30:07.58 -07:07:57.5 -- not an asteroid (will add it to exclusion list)
11:37:07.02 -05:06:09.2 -- not an asteroid (will add it to exclusion list)
11:36:21.98 -06:22:34.5 -- not an asteroid (will add it to exclusion list)
11:35:33.58 -06:23:51.4 -- not an asteroid (will add it to exclusion list)
11:37:32.95 -06:05:59.9 -- not an asteroid (will add it to exclusion list)
11:09:14.51 -04:27:50.8 -- asteroid (will NOT add it to exclusion list)
11:23:28.23 -03:23:03.2 -- asteroid (will NOT add it to exclusion list)
11:38:12.91 -04:52:15.2 -- not an asteroid (will add it to exclusion list)
11:37:12.39 -06:38:16.8 -- not an asteroid (will add it to exclusion list)
11:36:35.90 -06:54:18.8 -- not an asteroid (will add it to exclusion list)
11:35:37.50 -07:02:21.4 -- not an asteroid (will add it to exclusion list)
11:34:36.71 -07:02:11.8 -- not an asteroid (will add it to exclusion list)
11:35:45.71 -06:20:28.0 -- not an asteroid (will add it to exclusion list)
11:36:02.03 -05:40:52.8 -- not an asteroid (will add it to exclusion list)
11:35:58.57 -07:02:14.8 -- not an asteroid (will add it to exclusion list)
11:35:49.90 -06:25:45.2 -- not an asteroid (will add it to exclusion list)
11:36:12.54 -05:57:15.7 -- not an asteroid (will add it to exclusion list)
11:34:09.21 -06:32:15.3 -- not an asteroid (will add it to exclusion list)
11:34:17.70 -06:19:59.7 -- not an asteroid (will add it to exclusion list)
11:35:31.86 -05:34:43.2 -- not an asteroid (will add it to exclusion list)
11:36:40.28 -05:43:54.0 -- not an asteroid (will add it to exclusion list)
11:37:59.28 -06:08:18.2 -- not an asteroid (will add it to exclusion list)
11:35:08.45 -07:06:28.6 -- not an asteroid (will add it to exclusion list)
11:33:22.99 -06:41:22.5 -- not an asteroid (will add it to exclusion list)
11:35:49.30 -05:42:12.3 -- not an asteroid (will add it to exclusion list)
11:37:01.84 -06:53:25.7 -- not an asteroid (will add it to exclusion list)
11:36:08.91 -06:26:00.4 -- not an asteroid (will add it to exclusion list)
11:36:41.49 -06:25:11.2 -- not an asteroid (will add it to exclusion list)
11:35:21.37 -07:05:27.4 -- not an asteroid (will add it to exclusion list)
11:38:21.06 -04:05:24.8 -- not an asteroid (will add it to exclusion list)
11:37:19.12 -06:23:29.6 -- not an asteroid (will add it to exclusion list)
11:23:33.96 -06:19:03.8 -- asteroid (will NOT add it to exclusion list)
10:45:24.33 -02:31:15.1 -- asteroid (will NOT add it to exclusion list)
11:37:39.25 -04:55:24.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
11:30:07.58 -07:07:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:33:22.99 -06:41:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:09.21 -06:32:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:17.70 -06:19:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:26.60 -05:45:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:36.71 -07:02:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:53.45 -06:42:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:08.45 -07:06:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:09.35 -05:56:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:21.37 -07:05:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:21.85 -05:15:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:31.86 -05:34:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:33.58 -06:23:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:37.50 -07:02:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:42.27 -06:44:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:45.71 -06:20:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:47.37 -06:38:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:49.30 -05:42:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:49.90 -06:25:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:58.57 -07:02:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:02.03 -05:40:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:08.91 -06:26:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:12.54 -05:57:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:21.98 -06:22:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:35.90 -06:54:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:40.28 -05:43:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:41.49 -06:25:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:57.37 -06:06:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:01.84 -06:53:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:07.02 -05:06:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:12.39 -06:38:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:19.12 -06:23:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:32.95 -06:05:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:39.25 -04:55:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:59.28 -06:08:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:12.91 -04:52:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:21.06 -04:05:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:39.28 -03:51:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
11:30:07.58 -07:07:57.5 -- not a known variable star
11:33:22.99 -06:41:22.5 -- not a known variable star
11:34:09.21 -06:32:15.3 -- not a known variable star
11:34:17.70 -06:19:59.7 -- not a known variable star
11:34:26.60 -05:45:07.7 -- not a known variable star
11:34:36.71 -07:02:11.8 -- not a known variable star
11:34:53.45 -06:42:47.7 -- not a known variable star
11:35:08.45 -07:06:28.6 -- not a known variable star
11:35:09.35 -05:56:59.3 -- not a known variable star
11:35:21.37 -07:05:27.4 -- not a known variable star
11:35:21.85 -05:15:26.4 -- not a known variable star
11:35:31.86 -05:34:43.2 -- not a known variable star
11:35:33.58 -06:23:51.4 -- not a known variable star
11:35:37.50 -07:02:21.4 -- not a known variable star
11:35:42.27 -06:44:16.0 -- not a known variable star
11:35:45.71 -06:20:28.0 -- not a known variable star
11:35:47.37 -06:38:17.5 -- not a known variable star
11:35:49.30 -05:42:12.3 -- not a known variable star
11:35:49.90 -06:25:45.2 -- a known variable star
11:35:58.57 -07:02:14.8 -- not a known variable star
11:36:02.03 -05:40:52.8 -- a known variable star
11:36:08.91 -06:26:00.4 -- not a known variable star
11:36:12.54 -05:57:15.7 -- not a known variable star
11:36:21.98 -06:22:34.5 -- not a known variable star
11:36:35.90 -06:54:18.8 -- not a known variable star
11:36:40.28 -05:43:54.0 -- not a known variable star
11:36:41.49 -06:25:11.2 -- not a known variable star
11:36:57.37 -06:06:15.7 -- a known variable star
11:37:01.84 -06:53:25.7 -- not a known variable star
11:37:07.02 -05:06:09.2 -- not a known variable star
11:37:12.39 -06:38:16.8 -- a known variable star
11:37:19.12 -06:23:29.6 -- not a known variable star
11:37:32.95 -06:05:59.9 -- not a known variable star
11:37:39.25 -04:55:24.7 -- not a known variable star
11:37:59.28 -06:08:18.2 -- not a known variable star
11:38:12.91 -04:52:15.2 -- not a known variable star
11:38:21.06 -04:05:24.8 -- not a known variable star
11:38:39.28 -03:51:39.9 -- not a known variable star
Found 34 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
38 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
No ../exclusion_list_TTUQ2.txt so we are not updating exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= YES
The observatory MPC code is 500
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461093.76839170 -observatory 500
23:23:38.10 -01:55:54.9 Mercury (-0.1mag)
23:04:55.83 -07:26:52.3 Venus (-3.9mag)
21:43:07.30 -14:51:17.1 Mars (1.1mag)
07:06:04.59 +22:54:22.7 Jupiter (-2.5mag)
00:05:28.73 -01:44:11.0 Saturn (1.0mag)
03:39:59.89 +19:21:45.1 Uranus (5.7mag)
00:03:41.65 -01:01:32.3 Neptune (7.8mag)
20:29:07.79 -22:59:32.4 Pluto (14.5mag)
01:59:39.67 +16:49:00.4 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 22 02:51 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461093.76839170:
07:06:11.27 +22:54:11.4 Io (5.4mag)
07:06:17.42 +22:53:58.3 Europa (5.5mag)
07:05:57.54 +22:54:44.4 Ganymede (4.9mag)
07:06:25.12 +22:53:54.2 Callisto (6.2mag)
07:09:14.02 +23:10:42.7 Himalia (15.0mag)
07:06:08.48 +22:54:15.8 Thebe (15.9mag)
07:08:39.02 +23:19:15.2 Elara (17.0mag)
07:01:38.47 +24:02:17.6 Pasiphae (17.0mag)
07:15:05.47 +22:42:24.6 Carme (18.1mag)
00:05:40.52 -01:44:15.3 Titan (8.8mag)
00:05:34.40 -01:44:09.3 Rhea (10.1mag)
00:05:24.39 -01:45:31.3 Iapetus (11.5mag)
00:05:29.97 -01:44:14.5 Hyperion (14.8mag)
00:07:32.98 -01:31:11.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 22 02:52 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.76839170:
08:46:40.12 +24:30:48.7 JWST
13:36:50.05 +54:18:23.3 Chandra
16:38:37.40 -50:30:50.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 22 02:51 spacecraft.txt
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Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461093.76839170 at 500
16:59:54.84 -11:03:54.6 17.5mag 10P/Tempel 2
03:37:25.34 +28:58:13.1 18.0mag 123P/West-Hartley
08:23:28.03 +60:40:49.7 18.4mag 124P/Mrkos
21:19:57.26 -07:36:52.9 22.1mag 141P/Machholz
01:21:24.10 +11:56:46.7 17.7mag 145P/Shoemaker-Levy 5
11:02:52.51 +30:35:18.2 17.9mag 164P/Christensen
09:33:04.16 -33:51:30.0 18.0mag 195P/Hill
15:52:02.50 -06:35:14.0 19.2mag 210P/Christensen
18:17:23.20 -21:28:06.8 17.3mag 218P/LINEAR
16:21:45.74 -18:10:46.4 15.2mag 235P/LINEAR
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for periodic comet 240P/NEAT
15:17:45.87 +06:37:54.4 14.8mag 24P/Schaumasse
11:23:28.31 -03:22:59.1 17.4mag 29P/Schwassmann-Wachmann 1
07:03:47.01 +27:24:52.3 19.6mag 407P/PanSTARRS-Fuls
17:07:20.08 -11:19:11.1 17.6mag 40P/Vaisala 1
11:02:08.42 -08:51:29.7 16.6mag 43P/Wolf-Harrington
13:25:30.14 -05:50:00.9 20.0mag 489P/Denning
04:45:22.33 +19:21:16.3 0.0mag 493P/2024 Q2 (LONEOS)
06:04:25.90 +47:30:11.4 17.7mag 63P/Wild 1
23:14:50.15 -02:06:15.4 16.2mag 78P/Gehrels 2
20:01:55.96 -22:17:18.0 14.9mag 88P/Howell
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS designation for periodic comet P/2023 S1 (PanSTARRS) -- you may manually insert its ID in util/comets.sh
04:43:27.78 -72:35:30.6 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:48.99 +31:12:55.3 18.2mag C/2017 K2 (PanSTARRS)
20:06:42.07 -65:11:51.1 18.1mag C/2020 V2 (ZTF)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2021 G2 (ATLAS)
03:35:46.52 +24:36:50.6 15.8mag C/2022 N2 (PanSTARRS)
09:08:10.87 +29:50:08.0 15.3mag C/2022 QE78 (ATLAS)
08:35:38.46 -06:32:56.0 16.7mag C/2022 R6 (PanSTARRS)
23:53:10.86 +48:27:02.5 18.0mag C/2023 C2 (ATLAS)
09:51:00.21 -20:44:58.8 17.5mag C/2023 F3 (ATLAS)
20:34:59.12 +61:14:31.4 17.3mag C/2023 H5 (Lemmon)
19:34:30.93 -03:24:19.3 16.1mag C/2023 R1 (PANSTARRS)
02:48:57.63 +35:40:31.0 18.5mag C/2023 RS61 (PanSTARRS)
21:01:38.66 +81:20:05.4 18.0mag C/2023 X2 (Lemmon)
06:38:59.69 +63:49:23.0 17.3mag C/2024 A1 (ATLAS)
01:57:36.16 -24:28:17.9 11.2mag C/2024 E1 (Wierzchos)
11:44:53.22 -02:33:32.2 18.1mag C/2024 G2 (ATLAS)
19:28:25.64 +00:39:26.7 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.52 -01:41:58.5 17.7mag C/2024 G6 (ATLAS)
19:53:32.37 +03:16:23.3 15.6mag C/2024 J3 (ATLAS)
02:47:18.29 -31:33:10.0 15.4mag C/2024 T5 (ATLAS)
16:24:47.06 -58:16:30.1 15.6mag C/2025 A6 (Lemmon)
04:50:28.15 +62:11:45.8 16.7mag C/2025 J1 (Borisov)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2025 K1 (ATLAS)
15:56:38.61 -12:55:30.3 14.8mag C/2025 L1 (ATLAS)
02:20:20.00 -19:06:56.7 16.7mag C/2025 Q3 (ATLAS)
02:09:43.38 +17:17:23.7 21.2mag C/2025 R2 (SWAN)
22:20:48.37 +17:39:24.7 16.4mag C/2025 R3 (PANSTARRS)
21:46:08.63 -16:51:53.8 21.5mag C/2025 T1 (ATLAS)
03:05:58.52 -20:30:39.5 18.3mag C/2026 A1 (MAPS)
21:03:28.00 +20:58:46.3 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.8K Feb 22 02:53 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
-rw-r--r-- 1 apache apache 6.2K Feb 22 02:51 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
-rw-r--r-- 1 apache apache 187K Feb 22 02:51 tocp_transients_list.txt