This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S
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 22.2506 2461093.7506 11.90 11:36:39.89 -13:59:09.0
276.81008 45.05983 galactic Crt Second-epoch detections are separated by 2.7" and 3.8 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 3584938940603382912 | 11:36:39.22 -13:59:10.1 (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 3584938940603382912,2461093.7506,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3584938940603382912 20260222.2506 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:39.89 -13:59:09.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 10.56 11:34:03.19 -14:39:25.4
276.38267 44.18908 galactic Crt Second-epoch detections are separated by 2.1" and 4.5 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 3560825482375228288 | 11:34:02.60 -14:39:24.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8III 1988MSS...C04....0H HD 100520
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 3560825482375228288,2461093.7506,10.56,0.05,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 3560825482375228288 20260222.2506 10.56CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:03.19 -14:39:25.4 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 10.76 11:38:08.65 -13:11:34.4
276.82349 45.93041 galactic Crt Second-epoch detections are separated by 3.3" and 4.1 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 3585101084208763136 | 11:38:08.04 -13:11:34.9 (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!
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 3585101084208763136,2461093.7506,10.76,0.05,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 3585101084208763136 20260222.2506 10.76CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:08.65 -13:11:34.4 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 11.37 11:37:41.87 -14:09:45.7
277.23512 44.99824 galactic Crt Second-epoch detections are separated by 5.6" and 5.2 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 3584880013651825920 | 11:37:41.33 -14:09:43.1 (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 3584880013651825920,2461093.7506,11.37,0.05,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 3584880013651825920 20260222.2506 11.37CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:41.87 -14:09:45.7 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 11.57 11:34:43.37 -15:05:19.8
276.83330 43.86101 galactic Crt Second-epoch detections are separated by 1.2" and 4.4 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 3560799197175792512 | 11:34:42.72 -15:05:19.2 (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!
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 3560799197175792512,2461093.7506,11.57,0.05,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 3560799197175792512 20260222.2506 11.57CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:43.37 -15:05:19.8 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 11.82 11:37:46.95 -12:56:26.8
276.56077 46.12545 galactic Crt Second-epoch detections are separated by 8.8" 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 | Gaia DR3 3585301985599552256 | 11:37:46.52 -12:56:27.1 (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 3585301985599552256,2461093.7506,11.82,0.05,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
Gaia DR3 3585301985599552256 20260222.2506 11.82CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:46.95 -12:56:26.8 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.15 11:38:18.25 -14:28:37.6
277.60105 44.76758 galactic Crt Second-epoch detections are separated by 2.6" and 3.7 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 3572853452388350080 | 11:38:17.57 -14:28:38.2 (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!
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 3572853452388350080,2461093.7506,12.15,0.05,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 3572853452388350080 20260222.2506 12.15CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:18.25 -14:28:37.6 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2506 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:23.51 -13:21:01.0 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,14.34,0.05,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 20260222.2506 14.34CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:33:30.59 -14:56:53.1 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,14.29,0.05,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 20260222.2506 14.29CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:39:08.01 -07:58:29.6 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,14.10,0.05,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 20260222.2506 14.10CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:32.91 -13:06:04.1 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2506 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:09.42 -14:37:18.7 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,13.89,0.05,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
target 20260222.2506 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:39:03.40 -11:05:30.6 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,13.97,0.05,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
target 20260222.2506 13.97CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:47.71 -13:39:26.4 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.90 11:37:30.09 -13:39:15.0
276.88427 45.44523 galactic Crt Second-epoch detections are separated by 5.5" and 3.2 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 3584977870186666496 | 11:37:30.65 -13:39:17.3 (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 3584977870186666496,2461093.7506,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3584977870186666496 20260222.2506 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:30.09 -13:39:15.0 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,13.95,0.05,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 20260222.2506 13.95CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:03.22 -12:47:30.8 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,13.92,0.05,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 20260222.2506 13.92CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:17.13 -13:22:17.1 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,13.92,0.05,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 20260222.2506 13.92CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:48.36 -11:52:40.0 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.73 11:36:30.21 -13:18:27.1
276.36678 45.66367 galactic Crt Second-epoch detections are separated by 2.0" and 3.9 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 3585195195532628352 | 11:36:30.78 -13:18:26.7 (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 3585195195532628352,2461093.7506,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3585195195532628352 20260222.2506 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:30.21 -13:18:27.1 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.21 11:34:10.48 -14:03:32.8
276.07433 44.74584 galactic Crt Second-epoch detections are separated by 2.0" and 4.2 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 3560930004697275392 | 11:34:09.90 -14:03:34.6 (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 3560930004697275392,2461093.7506,13.21,0.05,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 3560930004697275392 20260222.2506 13.21CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:10.48 -14:03:32.8 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.85 11:37:26.61 -12:15:01.0
276.04180 46.72183 galactic Crt Second-epoch detections are separated by 3.5" and 3.8 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 3585420732855263360 | 11:37:27.03 -12:15:00.6 (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 3585420732855263360,2461093.7506,12.85,0.05,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 3585420732855263360 20260222.2506 12.85CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:26.61 -12:15:01.0 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.85 11:39:46.72 -09:32:41.4
275.13613 49.42036 galactic Crt Second-epoch detections are separated by 2.7" and 3.7 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 3588610794043894144 | 11:39:47.22 -09:32:39.3 (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 3588610794043894144,2461093.7506,12.85,0.05,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 3588610794043894144 20260222.2506 12.85CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:39:46.72 -09:32:41.4 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.30 11:39:14.87 -10:20:03.3
275.45973 48.64883 galactic Crt Second-epoch detections are separated by 3.4" and 4.4 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 3587015471391079808 | 11:39:14.36 -10:20:04.7 (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 3587015471391079808,2461093.7506,12.30,0.05,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 3587015471391079808 20260222.2506 12.30CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:39:14.87 -10:20:03.3 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.37 11:34:11.29 -13:58:17.1
276.02728 44.82699 galactic Crt Second-epoch detections are separated by 0.8" and 4.2 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 3561125202373302528 | 11:34:10.82 -13:58:19.7 (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 3561125202373302528,2461093.7506,12.37,0.05,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 3561125202373302528 20260222.2506 12.37CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:11.29 -13:58:17.1 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 11.72 11:37:26.61 -12:03:55.0
275.93030 46.89035 galactic Crt Second-epoch detections are separated by 2.3" and 4.4 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 3585428017119804416 | 11:37:26.09 -12:03:56.5 (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!
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 3585428017119804416,2461093.7506,11.72,0.05,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 3585428017119804416 20260222.2506 11.72CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:26.61 -12:03:55.0 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 10.77 11:39:18.26 -10:06:52.4
275.33959 48.85422 galactic Crt Second-epoch detections are separated by 0.9" and 4.1 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 3587028425012432640 | 11:39:18.66 -10:06:50.4 (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 3587028425012432640,2461093.7506,10.77,0.05,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 3587028425012432640 20260222.2506 10.77CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:39:18.26 -10:06:52.4 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 10.92 11:35:18.51 -13:48:53.1
276.28575 45.08197 galactic Crt Second-epoch detections are separated by 1.1" and 4.2 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 | Large-amplitude variable Gaia DR2 3584960243639038080 | 11:35:18.06 -13:48:54.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G6/8IV 1988MSS...C04....0H HD 100718
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
Large-amplitude variable Gaia DR2 3584960243639038080,2461093.7506,10.92,0.05,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
Large-amplitude variable Gaia DR2 3584960243639038080 20260222.2506 10.92CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:18.51 -13:48:53.1 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.17 11:36:50.82 -14:10:28.1
276.97467 44.90497 galactic Crt Second-epoch detections are separated by 1.9" and 3.7 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 3584886542000510464 | 11:36:50.25 -14:10:26.0 (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!
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 3584886542000510464,2461093.7506,12.17,0.05,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
Gaia DR3 3584886542000510464 20260222.2506 12.17CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:50.82 -14:10:28.1 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.19 11:35:22.14 -14:40:20.0
276.79688 44.30514 galactic Crt Second-epoch detections are separated by 2.6" and 4.4 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 3560816548843310464 | 11:35:21.51 -14:40:20.1 (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 3560816548843310464,2461093.7506,12.19,0.05,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 3560816548843310464 20260222.2506 12.19CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:22.14 -14:40:20.0 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.52 11:37:23.57 -15:07:57.6
277.67849 44.07822 galactic Crt Second-epoch detections are separated by 1.0" and 4.1 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 3548730751390337792 | 11:37:22.92 -15:07:59.2 (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!
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 3548730751390337792,2461093.7506,12.52,0.05,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 3548730751390337792 20260222.2506 12.52CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:23.57 -15:07:57.6 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.59 11:36:55.49 -14:39:31.2
277.27143 44.46875 galactic Crt Second-epoch detections are separated by 2.4" and 3.7 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 3548827405334341632 | 11:36:55.02 -14:39:30.4 (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 3548827405334341632,2461093.7506,12.59,0.05,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 3548827405334341632 20260222.2506 12.59CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:55.49 -14:39:31.2 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.80 11:37:05.54 -14:18:14.3
277.12473 44.81015 galactic Crt Second-epoch detections are separated by 0.6" and 4.0 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 3584871423717175680 | 11:37:04.97 -14:18:12.9 (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!
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 3584871423717175680,2461093.7506,12.80,0.05,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 3584871423717175680 20260222.2506 12.80CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:05.54 -14:18:14.3 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.78 11:35:58.25 -14:33:22.8
276.91766 44.46999 galactic Crt Second-epoch detections are separated by 7.0" 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 3560842284287400064 | 11:35:57.81 -14:33:21.6 (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 3560842284287400064,2461093.7506,12.78,0.05,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 3560842284287400064 20260222.2506 12.78CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:58.25 -14:33:22.8 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.94 11:39:28.39 -11:04:18.7
275.99486 48.00034 galactic Crt Second-epoch detections are separated by 1.5" and 4.1 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 3586719427885920640 | 11:39:27.71 -11:04:21.3 (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 3586719427885920640,2461093.7506,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3586719427885920640 20260222.2506 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:39:28.39 -11:04:18.7 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 12.85 11:33:27.53 -14:58:19.7
276.38091 43.84280 galactic Crt Second-epoch detections are separated by 2.6" and 4.5 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 3560723330873226240 | 11:33:26.92 -14:58:19.1 (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 3560723330873226240,2461093.7506,12.85,0.05,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 3560723330873226240 20260222.2506 12.85CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:33:27.53 -14:58:19.7 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.19 11:34:41.51 -14:51:05.4
276.68981 44.07482 galactic Crt Second-epoch detections are separated by 2.2" and 3.9 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 | Large-amplitude variable Gaia DR2 3560807443512633216 | 11:34:40.94 -14:51:04.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
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
Large-amplitude variable Gaia DR2 3560807443512633216,2461093.7506,13.19,0.05,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
Large-amplitude variable Gaia DR2 3560807443512633216 20260222.2506 13.19CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:41.51 -14:51:05.4 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.18 11:35:55.34 -13:57:47.5
276.56410 45.00747 galactic Crt Second-epoch detections are separated by 5.9" and 4.6 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 J173.9786-13.9629 | 11:35:54.88 -13:57:46.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J173.9786-13.9629,2461093.7506,13.18,0.05,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 J173.9786-13.9629 20260222.2506 13.18CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:55.34 -13:57:47.5 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.19 11:38:32.66 -13:50:57.9
277.32600 45.36729 galactic Crt Second-epoch detections are separated by 2.6" and 4.6 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 3584921932532650880 | 11:38:32.18 -13:50:58.6 (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 3584921932532650880,2461093.7506,13.19,0.05,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 3584921932532650880 20260222.2506 13.19CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:32.66 -13:50:57.9 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.46 11:38:32.15 -13:33:11.6
277.15546 45.63831 galactic Crt Second-epoch detections are separated by 3.6" and 3.6 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 3584983127226947200 | 11:38:31.74 -13:33:11.4 (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 3584983127226947200,2461093.7506,13.46,0.05,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 3584983127226947200 20260222.2506 13.46CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:32.15 -13:33:11.6 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.43 11:35:52.16 -15:04:16.9
277.17518 43.98853 galactic Crt Second-epoch detections are separated by 1.6" and 4.3 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 3548786963922261376 | 11:35:51.69 -15:04:16.2 (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!
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 3548786963922261376,2461093.7506,13.43,0.05,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 3548786963922261376 20260222.2506 13.43CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:35:52.16 -15:04:16.9 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.31 11:34:03.46 -15:02:33.4
276.60383 43.83785 galactic Crt Second-epoch detections are separated by 3.8" and 5.0 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 3560709277740258560 | 11:34:03.01 -15:02:31.9 (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!
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 3560709277740258560,2461093.7506,13.31,0.05,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 3560709277740258560 20260222.2506 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:03.46 -15:02:33.4 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.38 11:34:48.16 -14:11:39.7
276.34803 44.68547 galactic Crt Second-epoch detections are separated by 1.1" and 4.2 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 3560913232850569856 | 11:34:47.59 -14:11:41.2 (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!
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 3560913232850569856,2461093.7506,13.38,0.05,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
Gaia DR3 3560913232850569856 20260222.2506 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:48.16 -14:11:39.7 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.55 11:37:29.78 -14:06:12.4
277.13833 45.03310 galactic Crt Second-epoch detections are separated by 4.2" and 3.8 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 3584892207062236544 | 11:37:29.04 -14:06:11.4 (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 3584892207062236544,2461093.7506,13.55,0.05,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 3584892207062236544 20260222.2506 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:29.78 -14:06:12.4 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.51 11:38:40.13 -13:56:04.8
277.41344 45.30095 galactic Crt Second-epoch detections are separated by 2.0" and 4.1 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 3584908566594421376 | 11:38:39.33 -13:56:03.7 (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 3584908566594421376,2461093.7506,13.51,0.05,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 3584908566594421376 20260222.2506 13.51CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:40.13 -13:56:04.8 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2506 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:14.83 -14:57:18.6 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.34 11:38:41.31 -11:50:51.6
276.20641 47.21390 galactic Crt Second-epoch detections are separated by 2.0" and 4.5 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 | Large-amplitude variable Gaia DR2 3585811918476208128 | 11:38:40.83 -11:50:54.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
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
Large-amplitude variable Gaia DR2 3585811918476208128,2461093.7506,13.34,0.05,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
Large-amplitude variable Gaia DR2 3585811918476208128 20260222.2506 13.34CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:41.31 -11:50:51.6 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.46 11:34:58.99 -14:40:08.0
276.67587 44.27029 galactic Crt Second-epoch detections are separated by 2.7" and 4.4 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 3560828093715400576 | 11:34:58.41 -14:40:08.5 (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!
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 3560828093715400576,2461093.7506,13.46,0.05,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 3560828093715400576 20260222.2506 13.46CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:58.99 -14:40:08.0 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.49 11:38:24.32 -14:43:02.6
277.76523 44.55616 galactic Crt Second-epoch detections are separated by 1.0" and 4.0 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 3548817372290790528 | 11:38:23.88 -14:43:02.4 (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 3548817372290790528,2461093.7506,13.49,0.05,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 3548817372290790528 20260222.2506 13.49CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:24.32 -14:43:02.6 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.62 11:33:52.12 -14:36:01.0
276.29332 44.22244 galactic Crt Second-epoch detections are separated by 2.4" and 4.2 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 3560878705609963008 | 11:33:51.53 -14:36:00.8 (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 3560878705609963008,2461093.7506,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3560878705609963008 20260222.2506 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:33:52.12 -14:36:01.0 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.63 11:38:32.23 -11:26:48.1
275.91325 47.56427 galactic Crt Second-epoch detections are separated by 3.6" and 4.8 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 3586609545442595968 | 11:38:31.58 -11:26:46.7 (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 3586609545442595968,2461093.7506,13.63,0.05,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 3586609545442595968 20260222.2506 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:32.23 -11:26:48.1 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.72 11:37:55.43 -14:08:05.2
277.29053 45.04563 galactic Crt Second-epoch detections are separated by 4.8" and 3.8 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 3584880352952500224 | 11:37:54.56 -14:08:02.7 (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 3584880352952500224,2461093.7506,13.72,0.05,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 3584880352952500224 20260222.2506 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:55.43 -14:08:05.2 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 13.78 11:38:48.95 -13:54:40.7
277.44694 45.33649 galactic Crt Second-epoch detections are separated by 4.5" and 4.6 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 3584909013271022848 | 11:38:48.10 -13:54:41.4 (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 3584909013271022848,2461093.7506,13.78,0.05,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 3584909013271022848 20260222.2506 13.78CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:48.95 -13:54:40.7 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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 22.2506* 11 23 34.80 -06 19 03.5 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
VARIABLE_NAME,2461093.7506,13.91,0.05,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 20260222.2506 13.91CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:23:34.80 -06:19:03.5 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,13.94,0.05,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
target 20260222.2506 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:49.17 -12:52:41.1 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 14.35 11:36:33.63 -14:17:46.3
276.95404 44.76560 galactic Crt Second-epoch detections are separated by 4.0" and 4.8 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 J174.1382-14.2957 | 11:36:33.63 -14:17:46.3 (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!
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 J174.1382-14.2957,2461093.7506,14.35,0.05,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 J174.1382-14.2957 20260222.2506 14.35CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:33.63 -14:17:46.3 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2506 2461093.7506 14.23 11:37:05.30 -14:05:23.9
277.00245 45.00585 galactic Crt Second-epoch detections are separated by 8.5" and 4.9 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 J174.2702-14.0899 | 11:37:05.30 -14:05:23.9 (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!
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 J174.2702-14.0899,2461093.7506,14.23,0.05,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
ATO J174.2702-14.0899 20260222.2506 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:05.30 -14:05:23.9 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,14.38,0.05,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
target 20260222.2506 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:13.89 -14:16:00.1 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,14.29,0.05,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 20260222.2506 14.29CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:13.42 -12:48:11.3 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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
VARIABLE_NAME,2461093.7506,14.43,0.05,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 20260222.2506 14.43CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:21:22.79 -08:24:18.5 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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,2461093.7506,14.44,0.05,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 20260222.2506 14.44CV 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:24.43 -13:21:01.6 ;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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20_00sec_-14_90C_LIGHT_0198_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20_00sec_-14_90C_LIGHT_0197_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: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
First image: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Last image: 2461093.75089612 22.02.2026 06:01:07.425 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 102
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6897
Objects passed selection criteria: 6895
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: 6361.5
Average stars matched: 6129.75 (96.357 %)
Memory usage VmPeak: 112684 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 00:58:39 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: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
First image: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Last image: 2461093.75089612 22.02.2026 06:01:07.425 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 289
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
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: 22 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): 39726
Objects passed selection criteria: 39660
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: 37234.5
Average stars matched: 35365.2 (94.9798 %)
Memory usage VmPeak: 140296 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 01:01:12 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:
Crt-01-Q2b1x1
#######################################
########### Starting Crt-01-Q2b1x1 ###########
Processing Crt-01-Q2b1x1
server tau has sufficient free disk space available: 1082432 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1082432 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.png' -> 'transient_report/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits_preview.png'
Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
renamed 'Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.png' -> 'transient_report/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits_preview.png'
Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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= 822.9443
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 513.8013
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1516.4373
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 575.4074
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1513.2825
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 574.6818
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.8427
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat to cache
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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: 2461093.75036052
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits exists and is non-empty
Saving wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits to local_wcs_cache/
'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> 'local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
Saving wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits to local_wcs_cache/
'wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> 'local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits exists and is non-empty
Saving wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits to local_wcs_cache/
'wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits' -> 'local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits'
wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits exists and is non-empty
Saving wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits to local_wcs_cache/
'wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits' -> 'local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:34.149 -09:59:57.82
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:35.732 -10:00:04.40
Angular distance between the image centers 0.06 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 11:08:34.149 -09:59:57.82
Second-epoch second image center 11:08:35.732 -10:00:04.40
Angular distance between the image centers 0.00675 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits &> /tmp/tmp.qIoUX0pN52
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.N5jWzbypUM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits &> /tmp/tmp.k4CaAxwMJg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits &> /tmp/tmp.elwUx02bTW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
Found non-empty wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
The reference image (wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits) and catalog (wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat) found
'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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 3905 out of 6631 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.839875
a=0.000000 b=1.000000 c=22.839875
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.10
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.10
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 94 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
2.0 pix Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
2.4 pix Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
2.5 pix Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
Limiting magnitude estimates:
15.1 mag. Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
15.1 mag. Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
14.8 mag. Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
14.8 mag. Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.0 (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.qIoUX0pN52 (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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> 'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=466, passed=6631
Got 6631 stars (including 6155 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 6631 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 966 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits -region wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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.N5jWzbypUM (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/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> 'wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=470, passed=6561
Got 6561 stars (including 6079 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 6561 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 968 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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.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.k4CaAxwMJg (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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=621, passed=6190
Got 6190 stars (including 5566 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat
util/solve_plate_with_UCAC5 got 6190 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 972 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits -region wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.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.elwUx02bTW (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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=621, passed=6219
Got 6219 stars (including 5594 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat
util/solve_plate_with_UCAC5 got 6219 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 969 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 970 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits -region wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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 Crt-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out20376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20537.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_local.txt__out20322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20503.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 35s
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: 5s
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Considering the candidate 20322_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 20322_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 20344_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20344_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:35:38.78 -14:27:40.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20351_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 20351_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 20361_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 20361_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 20362_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20362_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:36:32.44 -12:13:16.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20376_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20376_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:39.80 -14:57:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 1.603 3548762362349707264 174.66566212451 -14.95919775033 10.0930 9.6970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20388_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 20388_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 20402_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 20402_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20407_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20407_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:09:50.20 -14:52:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.535 3563026017457880832 167.45936160092 -14.86661757227 11.7082 11.0938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20412_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20412_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:03:30.10 -10:59:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 0.332 3758390469000692224 165.87536062544 -10.98737954226 12.2343 11.9392 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20414_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20414_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:36.56 -09:21:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 0.344 3759214862203359488 166.90224524293 -09.35117837159 12.0905 11.9425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20415_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20415_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:05:16.02 -10:39:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 0.191 3758494961260910848 166.31669979637 -10.65998046765 11.9408 11.4482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20418_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20418_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:01:18.20 -10:03:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.566 3759523245151451520 165.32584139591 -10.05393482033 11.9397 11.4666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20422_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20422_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:03:43.52 -10:09:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 0.382 3758782066939231872 165.93122977002 -10.15169615029 12.0337 11.5889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20425_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20425_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:04:14.73 -10:05:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 0.697 3758737094337241600 166.06134563256 -10.09388578641 11.9870 11.4183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20427_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20427_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:01:59.34 -10:56:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 0.588 3758576664422914688 165.49740872063 -10.93960424207 12.0183 11.5751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20430_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20430_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:08:22.23 -11:32:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.322 3566221473126836480 167.09256849706 -11.54137424477 12.0581 11.5645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20431_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20431_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:04:49.15 -10:27:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 0.633 3758689158206693760 166.20472384683 -10.45452394679 12.1479 11.6816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20432_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20432_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:04:01.78 -10:35:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.525 3758680430833149824 166.00729047857 -10.59768797695 12.0556 11.4792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20435_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20435_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:06:42.28 -10:10:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.943 3758910778519618560 166.67640413695 -10.17428481284 12.0253 11.3259 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20437_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20437_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:02:10.17 -10:14:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.454 3758754682227754752 165.54234923234 -10.24576248444 11.8696 11.0158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20439_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20439_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:06:18.95 -11:12:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.096 3758400914361396992 166.57893118788 -11.21278016900 12.1650 11.7239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20440_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20440_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:05:50.11 -09:43:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.504 3759177551823709312 166.45868331464 -09.72550715989 12.2200 11.7878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20441_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20441_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:11:56.53 -09:19:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.550 3759083165622142336 167.98569352180 -09.31952575005 12.4736 11.9796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20442_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20442_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:13.83 -08:31:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.589 3760136321667053568 166.80748737137 -08.51847957966 12.1352 11.6645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20445_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20445_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:06:23.88 -12:00:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 0.432 3566088913255587968 166.59956489059 -12.00256479157 11.8297 10.9139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20447_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20447_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:10:07.21 -09:40:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 0.741 3759046435061788800 167.52983775443 -09.67265573341 12.2459 11.7531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20448_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20448_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:11:50.37 -11:02:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.394 3566591390069582976 167.95978765667 -11.04779298130 12.1991 11.7186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20449_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20449_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:13:41.39 -10:48:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.292 3566619217162260480 168.42239525406 -10.80535795599 12.1853 11.6734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20452_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20452_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:38.46 -09:59:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.850 3758920090008320384 166.91037507242 -09.98785402162 12.1423 11.5096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20453_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20453_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:54:46.79 -11:08:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.457 3757852571592713344 163.69508754981 -11.13574722911 12.0594 11.6103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20454_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 20454_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 20455_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20455_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:29.39 -11:43:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.690 3566124338145857152 166.87264623634 -11.71691804191 12.1890 11.7280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20456_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20456_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:03:54.66 -10:34:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.921 3758683351410910976 165.97771691455 -10.58302394022 12.1004 11.4069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20457_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20457_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:12:17.23 -09:42:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.266 3758990733630035200 168.07177218491 -09.70784534942 12.1453 11.5322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20458_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20458_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:15:07.41 -09:05:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.399 3783056844138873728 168.78098305846 -09.09514078131 12.1851 11.7306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20460_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20460_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:55.45 -10:39:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.657 3758461318781207680 166.98119246924 -10.66447672637 12.2454 11.7892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20462_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20462_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:57:13.66 -09:04:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.344 3759882368841188992 164.30701326053 -09.07146489886 12.0992 11.6610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20463_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20463_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:05:02.11 -10:51:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.484 3758473589503640192 166.25872532894 -10.85141011641 12.3230 11.8318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20464_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20464_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:05:08.28 -11:28:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.187 3758297388469470848 166.28455054254 -11.47331797910 12.2491 11.7819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20466_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20466_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:19:35.05 -08:34:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.280 3783201915250230272 169.89612004501 -08.57938330147 12.1393 11.6521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20467_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20467_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:58:21.68 -10:45:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.537 3758629750219102848 164.59046214095 -10.76303230111 12.2039 11.7943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20469_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20469_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:06:23.37 -11:38:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.700 3566139933171215104 166.59757264773 -11.63793577492 12.2424 11.7889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20470_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20470_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:08:39.18 -09:20:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.273 3759258395992302336 167.16330816233 -09.34027193982 12.2420 11.7223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20471_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20471_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:05:06.60 -09:01:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.508 3759986483143761664 166.27762844086 -09.02595077201 12.3353 12.0100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20474_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20474_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:11:53.18 -11:57:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.390 3565949206559771008 167.97155775067 -11.96128342163 12.1664 11.6699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20475_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20475_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:16:37.60 -10:52:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.372 3566506414140556544 169.15665139964 -10.87540783943 12.1973 11.7945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20477_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20477_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:04:42.35 -10:53:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.677 3758483274654259840 166.17661960885 -10.88798201438 12.2394 11.7484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20478_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20478_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:05:13.62 -08:29:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.900 3760160682721555840 166.30700270662 -08.48640911254 12.2142 11.7337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20479_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20479_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:04:26.46 -11:11:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.088 3758369509560299392 166.11026254431 -11.18754888867 12.0969 11.3542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20480_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20480_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:09:31.31 -11:04:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.630 3566267579599162496 167.38061463625 -11.08077713980 12.3038 11.8144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20481_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20481_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:11:10.53 -07:50:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.447 3784198004065438080 167.79377652984 -07.84200670813 12.2587 11.8460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20482_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20482_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:05:54.21 -12:28:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.691 3566012321102928128 166.47604829577 -12.47971475023 12.1936 11.6395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20483_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20483_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:04:29.33 -08:55:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.791 3760002559205448448 166.12242695195 -08.93318220033 12.1921 11.6576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20486_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20486_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:56:47.28 -11:01:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.602 3757867754300913152 164.19716927147 -11.03284321400 12.1671 11.7582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20488_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20488_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:21.23 -11:03:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.076 3758410264505909760 166.83845775787 -11.06064561965 12.3103 11.7727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20489_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20489_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:17:10.87 -10:07:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.109 3566761638277769472 169.29531449849 -10.12315914511 12.2319 11.7333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20490_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20490_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:12:11.20 -12:14:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.278 3565893780005787264 168.04672312631 -12.24983191487 12.2149 11.7543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20491_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20491_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:58:30.20 -09:06:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.114 3759832448436757504 164.62586152211 -09.10759824450 12.1503 11.6949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20494_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20494_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:11:58.84 -09:39:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.470 3758992146675230208 167.99529779247 -09.65442563071 12.2243 11.5835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20496_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20496_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:09:09.09 -09:59:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.486 3758930157411666688 167.28778268879 -09.98968306620 12.2537 11.6001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20497_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20497_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:36.08 -07:56:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.448 3784225625000012288 166.90044890431 -07.93477110251 12.2050 11.7646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20498_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20498_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:54.26 -11:40:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.450 3566217964137573120 166.97619557741 -11.66877382550 12.3053 11.8535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20501_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20501_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:58.04 -10:26:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.698 3758887723134993280 166.99201204813 -10.44402905373 12.2967 11.6452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20502_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20502_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:09:51.50 -11:20:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.471 3566208004109436544 167.46471556739 -11.34689841083 12.1062 11.2992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20503_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 20503_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 20504_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20504_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:00:14.12 -10:38:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.630 3758658513615626624 165.05875719669 -10.64893601324 12.2548 11.8012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20505_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20505_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:59:21.93 -09:27:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.722 3759622265621426304 164.84157257042 -09.45939764942 12.2066 11.7097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20506_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20506_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:11:26.43 -09:48:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.981 3758983483725674496 167.85990178002 -09.80246636803 12.3880 11.9968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20507_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20507_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:12:26.38 -11:12:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.323 3566576714165273472 168.10999812022 -11.20229263935 11.8753 10.8837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20508_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20508_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:03:51.35 -10:52:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.509 3758393290795243648 165.96409121660 -10.88213792511 12.2674 11.6710 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20509_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20509_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:11:57.54 -10:55:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.454 3566602037292446080 167.98977020928 -10.91809688549 12.2780 11.7202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20510_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20510_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:08:41.20 -08:32:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.449 3759370958495448064 167.17158913428 -08.54393181990 12.3200 11.8618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20511_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20511_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:05:13.31 -10:54:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.609 3758472039019813888 166.30561884142 -10.90199381954 12.3613 11.9357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20512_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20512_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:11:52.31 -08:35:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.450 3783335986949132032 167.96802355607 -08.58583749242 12.1782 11.5477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20514_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20514_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:09:05.74 -08:44:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.594 3759364537519744000 167.27406793148 -08.74026375333 12.2759 11.6806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20515_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20515_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:06:34.18 -10:05:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 1.125 3759100169397424256 166.64267229744 -10.08690738650 12.3272 11.8446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20516_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20516_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:08:45.20 -07:42:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.326 3784236177734680960 167.18824997942 -07.70976812535 12.2924 11.8018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20517_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20517_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:42.34 -11:30:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.350 3566225557639153280 166.92641270544 -11.50081948998 12.3853 11.9258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20518_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20518_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:01:37.90 -08:52:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.192 3760039358485895296 165.40792873501 -08.87044074201 12.2591 11.8098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20519_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20519_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:02:45.19 -11:30:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.766 3758328552752160640 165.68820654792 -11.51410975522 12.2179 11.6126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20520_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20520_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:10:46.29 -07:44:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.476 3784211571866081920 167.69291259398 -07.73403981300 12.2737 11.8362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20521_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20521_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:11:53.18 -09:47:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.737 3758988568966952704 167.97168942031 -09.78982398128 12.1806 11.3969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20523_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20523_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:10:22.68 -10:17:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.464 3758858556012929664 167.59460510210 -10.29950639019 12.3641 11.8507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20525_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20525_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:08:19.19 -10:27:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.615 3758840895107333376 167.08012887224 -10.46299568014 12.3149 11.6070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20526_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20526_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:57:54.55 -10:13:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.230 3759461771283269504 164.47734262145 -10.22007151677 12.2486 11.8045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20527_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20527_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:56:28.35 -10:06:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.153 3759478130814765440 164.11812419270 -10.10340186285 12.2352 11.8165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20528_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20528_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:59:46.89 -10:04:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.911 3759443938579481856 164.94513384921 -10.08000420279 12.1989 11.5397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20529_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20529_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:08:31.39 -08:23:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.706 3760132610815620736 167.13096113165 -08.39056497676 12.2390 11.7017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20531_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20531_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:04:45.29 -08:56:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.105 3759999844786117632 166.18901888182 -08.94040560782 12.3596 11.8926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20536_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20536_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:53:12.90 -10:39:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.637 3757928399239628288 163.30379959647 -10.65996871292 12.1423 11.6555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20537_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20537_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:14:04.45 -11:06:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.684 3566416357266709120 168.51873512071 -11.10651836052 12.2952 11.7908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20538_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20538_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:12:56.20 -10:00:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.512 3758966578734401664 168.23428796553 -10.00660511289 12.3342 11.7020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20539_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 20539_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:06:34.32 -09:10:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.732 3759232012009042048 166.64295894892 -09.18243968791 12.3234 11.8290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 41s
Prepared the HTML report for the field Crt-01-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 ####
11:36:39.89 -13:59:09.0
11:34:03.19 -14:39:25.4
11:38:08.65 -13:11:34.4
11:37:41.87 -14:09:45.7
11:34:43.37 -15:05:19.8
11:37:46.95 -12:56:26.8
11:38:18.25 -14:28:37.6
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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat to cache
SExtractor catalog cache: saved Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Creating symlink local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Creating symlink local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
Creating symlink local_wcs_cache/wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits exists and is non-empty
wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits exists and is non-empty
wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:34.149 -09:59:57.82
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:35.732 -10:00:04.40
Angular distance between the image centers 0.06 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 11:08:34.149 -09:59:57.82
Second-epoch second image center 11:08:35.732 -10:00:04.40
Angular distance between the image centers 0.00675 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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits &> /tmp/tmp.69njlpmxlk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.Ul7OybEnUC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits &> /tmp/tmp.ZuQO8xdP8t
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits &> /tmp/tmp.W6sR5IWHio
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
Found non-empty wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
The reference image (wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits) and catalog (wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat) found
'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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 4023 out of 40110 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.714876
a=0.000000 b=1.000000 c=22.714876
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 179 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
1.9 pix Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
2.3 pix Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
2.3 pix Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
Limiting magnitude estimates:
15.2 mag. Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
15.3 mag. Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
15.0 mag. Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
15.0 mag. Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.69njlpmxlk (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/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> 'wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1646, passed=40101
Got 40101 stars (including 38397 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 40101 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 965 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: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 965 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: 0.29"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits -region wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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.Ul7OybEnUC (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/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> 'wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1596, passed=40499
Got 40499 stars (including 38842 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 40499 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 968 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: 0.32"
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 968 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: 0.31"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.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.ZuQO8xdP8t (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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2109, passed=34664
Got 34664 stars (including 32518 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat
util/solve_plate_with_UCAC5 got 34664 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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits -region wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-00-21_20.00sec_-14.90C_LIGHT_0197.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.W6sR5IWHio (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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
WCS-calibrated image found: wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
Checking if the catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat corresponding to the image wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits
WCS catalog name: wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2208, passed=34762
Got 34762 stars (including 32515 good ones) from the SExtractor catalog wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat
util/solve_plate_with_UCAC5 got 34762 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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Crt-01-Q2b1x1_000149_TTUQ2b1x1_2376_XeVtW11S/Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits -region wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198.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 Crt-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53597.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out54160.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out54583.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out53248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54817.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 118s
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: 37s
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Considering the candidate 53248_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53248_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53250_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53250_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:32:22.70 -13:38:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 3.402 3561196189592688384 173.09362130132 -13.64785930599 13.4394 12.9591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53251_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53251_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 53253_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53253_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:36:35.41 -12:00:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.423 3586181350086866944 174.14783247904 -12.00591995058 13.1613 12.5247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53254_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53254_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:32:09.31 -13:33:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 3.229 3561200690718339072 173.03793422652 -13.55735883430 13.2711 12.7464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53258_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53258_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:30:11.58 -14:35:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.524 3560981372508118656 172.54868370372 -14.59502888332 13.2714 12.7121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53263_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53263_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:34:52.46 -12:36:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 4.737 3585381494033968512 173.71975544449 -12.60746047534 13.3077 12.7823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53265_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53265_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53268_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53268_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:34:05.74 -13:54:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 4.430 3561126439323885568 173.52517754973 -13.90862776588 13.0207 12.3890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53269_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53269_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:30:09.39 -14:52:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 5.180 3560761710700782464 172.54060533057 -14.87506849981 13.1075 12.4686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53270_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53270_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:02:52.40 -05:31:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.411 3788023033219859584 165.71863976625 -05.52719041016 14.3593 13.7159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53271_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53271_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:29:45.02 -14:38:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.782 3560957492489945216 172.43807690581 -14.64679740284 13.1947 12.5203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53272_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53272_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53273_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53273_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:33:53.35 -14:34:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 3.231 3560878739969703552 173.47316124311 -14.57810475353 12.7838 12.1920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53274_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53274_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:32:42.85 -14:37:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 5.715 3560875544513982208 173.17994753582 -14.61687627056 13.0185 12.4911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53275_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53275_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:32:38.87 -14:04:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 3.570 3561097852021521280 173.16292247958 -14.07017016113 13.2057 12.7992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53276_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53276_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:30:09.16 -14:28:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.018 3560995803598242176 172.53787612815 -14.47305574657 13.0759 12.4409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.018#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53277_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53277_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 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 53279_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53279_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:31:41.19 -14:50:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 4.497 3560772224780776960 172.92033526073 -14.83978475383 12.7815 12.1619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53280_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53280_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:08.27 -12:16:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 3.005 3585415029138691584 174.28530333994 -12.26712849301 12.9662 12.4991 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#
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Considering the candidate 53282_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53282_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 53284_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53284_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:43:36.52 -10:27:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.020 3760773767828871680 160.90245234291 -10.46457346947 13.9823 13.4769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53285_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53285_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:30:16.93 -14:18:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 3.187 3561006936153484800 172.57145497396 -14.30307247253 13.0376 12.3595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53289_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53289_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53293_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53293_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53295_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53295_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 53297_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53297_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:12:06.24 -07:37:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 2.131 3784295517003075840 168.02552114062 -07.62479831931 14.0431 13.5808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53298_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53298_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:07.33 -13:30:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 3.267 3584992610514397440 174.28146414349 -13.51358433339 12.4731 11.7090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53299_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53299_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 53300_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53300_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 53302_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53302_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53303_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53303_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53305_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53305_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:49.76 -12:29:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.512 3585354208104368000 174.70776262349 -12.48383227386 12.5348 11.7774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53307_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53307_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 53308_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53308_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 53310_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53310_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 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 53312_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53312_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53313_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53313_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:31:25.97 -14:49:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.315 3560784078890511744 172.85697100845 -14.83010311048 12.5588 11.9489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53314_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53314_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:07.07 -12:05:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 4.607 3585799029277684224 174.52818225734 -12.08789477495 12.6923 12.1836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53315_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53315_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:36:44.32 -13:12:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 4.387 3585197738153272064 174.18345803543 -13.20162233909 12.5422 11.8799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53316_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53316_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:48.27 -12:14:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.427 3585781647546686976 174.70043539873 -12.23368213631 12.3493 11.6987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53318_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53318_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53319_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53319_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 53320_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53320_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 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 53321_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53321_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:31:32.95 -13:38:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.638 3561192719259027712 172.88889551097 -13.64578978570 12.7828 12.2057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53323_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53323_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:34:55.72 -14:17:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.694 3560908937882512384 173.73202980624 -14.28730467260 12.4225 11.9804 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#
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Considering the candidate 53325_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53325_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:33:32.83 -13:35:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 3.408 3585169150850805120 173.38775119755 -13.58969918640 12.8253 12.2997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53327_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53327_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53329_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53329_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 53330_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53330_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53331_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53331_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:35:49.25 -12:42:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.189 3585365929072495488 173.95505869577 -12.71125697567 12.5101 11.8652 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53332_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53332_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 53334_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53334_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53336_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53336_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 53338_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53338_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 53339_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53339_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 53340_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53340_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:13.78 -12:12:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.687 3585424065749885952 174.30817719471 -12.21484802478 12.5049 12.0013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53341_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53341_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 53342_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53342_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:32:57.36 -13:56:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.646 3561123896703212160 173.23974059793 -13.94515246694 12.6552 12.1445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53343_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53343_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 53344_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53344_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 53347_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53347_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 53348_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53348_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 53350_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53350_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:28.32 -11:12:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 5.473 3586669193948365952 174.61646009529 -11.20028204158 12.3091 11.8569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53351_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53351_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:36:13.28 -12:41:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.714 3585365516755671936 174.05637776084 -12.69345004282 12.2192 11.6070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53353_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53353_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 53354_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53354_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:31:12.72 -14:30:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.562 3560985976713118848 172.80206578537 -14.50687342764 12.3268 11.7619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53355_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53355_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:47:14.62 -08:44:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.027 3761609632889262464 161.81119164345 -08.74355872594 13.2157 12.6664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53356_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53356_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 53357_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53357_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 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 53359_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53359_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 53361_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53361_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 53362_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53362_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 53363_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53363_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53364_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53364_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:13:38.94 -05:15:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.201 3785233361768463488 168.41243830979 -05.26255730022 13.3192 12.7358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53365_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53365_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 53367_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53367_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 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 53368_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53368_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53369_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53369_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 53372_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53372_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53374_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53374_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:58.17 -12:53:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 5.154 3585302535355368960 174.49382658304 -12.89763458266 11.2998 10.6522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53376_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53376_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:09.13 -11:43:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 5.568 3586575598021018496 174.28647087830 -11.71907996680 11.3744 10.7236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53377_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53377_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:39:48.07 -09:44:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.379 3588556574376742400 174.94936001786 -09.74755535622 11.3441 10.7395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53380_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53380_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 53382_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53382_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53383_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53383_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53384_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53384_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:35:49.98 -12:44:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.668 3585364172428417792 173.95756621002 -12.73807318363 10.9050 10.2760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53385_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53385_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:19:02.66 -07:41:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.486 3783684910092368384 169.76115458511 -07.69144851134 11.8896 11.2776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53386_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53386_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 53387_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53387_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53388_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53388_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 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 53389_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53389_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53390_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53390_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:36:50.06 -12:21:03.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.82, MAG_FAINT_SEARCH_LIMIT=10.80)
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Considering the candidate 53407_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53407_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:35:43.29 -14:35:36.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53410_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53410_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:35:38.74 -14:27:40.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53412_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53412_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:42.77 -14:40:03.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53431_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53431_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53432_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53432_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:08.60 -13:11:33.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53471_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53471_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:39.90 -14:57:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.852 3548762362349707264 174.66566212451 -14.95919775033 10.0930 9.6970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53473_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53473_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:42.14 -14:09:45.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53493_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53493_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:34:43.39 -15:05:20.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53531_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53531_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:33:28.52 -15:03:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 4.503 3560708831063630848 173.36758757527 -15.05543563662 10.7864 10.3678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53537_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53537_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53543_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53543_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:47.12 -12:56:25.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53555_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53555_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:46:05.74 -04:44:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.981 3777163672267828096 161.52418620671 -04.73396317099 11.4046 10.7755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53560_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53560_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:34.98 -15:02:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 2.086 3548801566811119616 174.39521449245 -15.04673855359 10.7934 10.3974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53569_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53569_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:18.30 -14:28:37.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53571_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53571_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53597_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53597_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:33:32.11 -14:50:40.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)
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Considering the candidate 53607_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53607_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:58.65 -13:31:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.619 3584985085731730688 174.49397380663 -13.53119745252 11.2093 10.7278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53628_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53628_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53630_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53630_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53650_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53650_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 53667_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53667_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:28.85 -13:50:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.770 3584922203113824512 174.61892118824 -13.83739298152 10.9825 10.3095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53705_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53705_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53719_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53719_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53721_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53721_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53724_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53724_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53771_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53771_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:36:51.33 -14:43:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.317 3548825962225327616 174.21298381211 -14.72311904065 11.6774 11.1672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53772_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53772_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:35.77 -13:51:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.326 3584921176618406272 174.64809356166 -13.86606097749 11.6662 11.1984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53829_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53829_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53845_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53845_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53857_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53857_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:32.52 -15:06:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.879 3548751229794468096 174.63502451355 -15.11358502436 11.5126 10.8919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53864_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53864_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:29:13.58 -05:22:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.413 3785932208780215040 172.30696394506 -05.37789762219 13.1210 12.6226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53869_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53869_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53901_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53901_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53922_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 53922_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:57.18 -13:50:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.397 3584924268994808832 174.48682348779 -13.83442681953 12.0169 11.5093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53929_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53929_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53942_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53942_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53943_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53943_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53963_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53963_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53968_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53968_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53969_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53969_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53980_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53980_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 53981_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 53981_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 54001_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54001_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:53:08.92 -14:38:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.823 3557837830107491840 163.28732731482 -14.63605468336 13.3415 12.6715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54021_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54021_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 54023_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54023_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:16.97 -14:22:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 5.715 3572858224094923648 174.56906957766 -14.36676946002 12.0809 11.5580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54053_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54053_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:19:30.35 -08:24:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.911 3783213180948774784 169.87641003773 -08.40964030879 13.8772 13.1314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54057_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54057_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:00:15.93 -12:40:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.574 3756610879367666048 165.06646360281 -12.66706060206 13.9248 13.4329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54068_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54068_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:19:40.69 -06:40:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.908 3784089186773964288 169.91934901528 -06.67649766458 13.5879 13.1701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54108_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54108_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 54127_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54127_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 54138_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54138_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:37:36.82 -13:33:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 3.868 3584985429329112192 174.40234288024 -13.56324523842 12.5771 12.0688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54160_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54160_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:30.44 -10:52:11.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)
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Considering the candidate 54162_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54162_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 54180_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54180_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:34:55.53 -14:44:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.741 3560814414242266880 173.73030591612 -14.73944997081 12.3216 11.6665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54189_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54189_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 54210_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54210_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 54261_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54261_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
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Considering the candidate 54275_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54275_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:44.23 -13:48:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.620 3584927979846607360 174.68354239856 -13.80548517688 12.3456 11.6885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54276_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54276_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:09.76 -14:40:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 4.152 3548818677960849408 174.53947732376 -14.66739319840 12.7862 12.3414 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54277_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54277_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:59.84 -12:52:43.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54294_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54294_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54296_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54296_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54330_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54330_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 54334_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54334_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:05:34.02 -11:03:50.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54348_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54348_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:41:51.37 -13:21:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.456 3751164620317744512 160.46371747678 -13.35905258317 13.8622 13.3646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54350_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54350_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:22:26.37 -07:06:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.997 3783814515025421824 170.60980746912 -07.11378695655 14.3736 13.8212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54363_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54363_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:09:48.15 -11:55:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.449 3566149455115282560 167.45076754574 -11.93103918396 14.4349 13.9646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54392_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54392_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54432_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54432_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:32:23.73 -05:36:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.436 3785855036807984384 173.09883926080 -05.60805090035 13.8362 13.3200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54436_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54436_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 10:40:53.76 -12:11:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 0.793 3751494508165763072 160.22384593563 -12.19878356988 14.0020 13.5274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54488_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54488_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54491_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54491_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:07:20.05 -08:49:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.510 3759341688293691008 166.83355942858 -08.83313720041 14.8041 14.4432 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 54493_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54493_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54499_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54499_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54507_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54507_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:15.87 -13:18:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.431 3585094933815599744 174.56556229665 -13.31467293332 12.9597 12.3321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54524_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54524_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 54560_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54560_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:24:44.08 -09:19:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 3.148 3590705741650881152 171.18285941701 -09.31811093294 14.8050 14.1498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54583_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54583_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:04:38.03 -07:02:48.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54598_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54598_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54632_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54632_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:38:25.13 -14:22:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 4.734 3572857506837099136 174.60339006625 -14.36976925768 13.0244 12.5702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54681_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54681_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:03:15.52 -11:16:08.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54692_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54692_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54750_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54750_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54817_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
Preparing report for the candidate 54817_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54935_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 54935_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
**** FOUND 11:31:35.53 -08:01:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 2.701 3592774369699413760 172.89732817702 -08.02252526457 14.5433 13.9710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31535_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198
The candidate 31535_Crt-01-Q2b1x1_2026-02-22_00-01-07_20.00sec_-14.90C_LIGHT_0198 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 161s
Prepared the HTML report for the field Crt-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:36:39.89 -13:59:09.0
11:34:03.19 -14:39:25.4
11:38:08.65 -13:11:34.4
11:37:41.87 -14:09:45.7
11:34:43.37 -15:05:19.8
11:37:46.95 -12:56:26.8
11:38:18.25 -14:28:37.6
11:37:23.51 -13:21:01.0
11:33:30.59 -14:56:53.1
11:39:08.01 -07:58:29.6
11:36:32.91 -13:06:04.1
11:34:09.42 -14:37:18.7
11:39:03.40 -11:05:30.6
11:34:47.71 -13:39:26.4
11:37:30.09 -13:39:15.0
11:37:03.22 -12:47:30.8
11:35:17.13 -13:22:17.1
11:35:48.36 -11:52:40.0
11:36:30.21 -13:18:27.1
11:34:10.48 -14:03:32.8
11:37:26.61 -12:15:01.0
11:39:46.72 -09:32:41.4
11:39:14.87 -10:20:03.3
11:34:11.29 -13:58:17.1
11:37:26.61 -12:03:55.0
11:39:18.26 -10:06:52.4
11:35:18.51 -13:48:53.1
11:36:50.82 -14:10:28.1
11:35:22.14 -14:40:20.0
11:37:23.57 -15:07:57.6
11:36:55.49 -14:39:31.2
11:37:05.54 -14:18:14.3
11:35:58.25 -14:33:22.8
11:39:28.39 -11:04:18.7
11:33:27.53 -14:58:19.7
11:34:41.51 -14:51:05.4
11:35:55.34 -13:57:47.5
11:38:32.66 -13:50:57.9
11:38:32.15 -13:33:11.6
11:35:52.16 -15:04:16.9
11:34:03.46 -15:02:33.4
11:34:48.16 -14:11:39.7
11:37:29.78 -14:06:12.4
11:38:40.13 -13:56:04.8
11:34:14.83 -14:57:18.6
11:38:41.31 -11:50:51.6
11:34:58.99 -14:40:08.0
11:38:24.32 -14:43:02.6
11:33:52.12 -14:36:01.0
11:38:32.23 -11:26:48.1
11:37:55.43 -14:08:05.2
11:38:48.95 -13:54:40.7
11:23:34.80 -06:19:03.5
11:38:49.17 -12:52:41.1
11:36:33.63 -14:17:46.3
11:37:05.30 -14:05:23.9
11:38:13.89 -14:16:00.1
11:36:13.42 -12:48:11.3
11:21:22.79 -08:24:18.5
11:37:24.43 -13:21:01.6
########### Completed Crt-01-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 ####
11:36:39.89 -13:59:09.0
11:34:03.19 -14:39:25.4
11:38:08.65 -13:11:34.4
11:37:41.87 -14:09:45.7
11:34:43.37 -15:05:19.8
11:37:46.95 -12:56:26.8
11:38:18.25 -14:28:37.6
11:37:23.51 -13:21:01.0
11:33:30.59 -14:56:53.1
11:39:08.01 -07:58:29.6
11:36:32.91 -13:06:04.1
11:34:09.42 -14:37:18.7
11:39:03.40 -11:05:30.6
11:34:47.71 -13:39:26.4
11:37:30.09 -13:39:15.0
11:37:03.22 -12:47:30.8
11:35:17.13 -13:22:17.1
11:35:48.36 -11:52:40.0
11:36:30.21 -13:18:27.1
11:34:10.48 -14:03:32.8
11:37:26.61 -12:15:01.0
11:39:46.72 -09:32:41.4
11:39:14.87 -10:20:03.3
11:34:11.29 -13:58:17.1
11:37:26.61 -12:03:55.0
11:39:18.26 -10:06:52.4
11:35:18.51 -13:48:53.1
11:36:50.82 -14:10:28.1
11:35:22.14 -14:40:20.0
11:37:23.57 -15:07:57.6
11:36:55.49 -14:39:31.2
11:37:05.54 -14:18:14.3
11:35:58.25 -14:33:22.8
11:39:28.39 -11:04:18.7
11:33:27.53 -14:58:19.7
11:34:41.51 -14:51:05.4
11:35:55.34 -13:57:47.5
11:38:32.66 -13:50:57.9
11:38:32.15 -13:33:11.6
11:35:52.16 -15:04:16.9
11:34:03.46 -15:02:33.4
11:34:48.16 -14:11:39.7
11:37:29.78 -14:06:12.4
11:38:40.13 -13:56:04.8
11:34:14.83 -14:57:18.6
11:38:41.31 -11:50:51.6
11:34:58.99 -14:40:08.0
11:38:24.32 -14:43:02.6
11:33:52.12 -14:36:01.0
11:38:32.23 -11:26:48.1
11:37:55.43 -14:08:05.2
11:38:48.95 -13:54:40.7
11:23:34.80 -06:19:03.5
11:38:49.17 -12:52:41.1
11:36:33.63 -14:17:46.3
11:37:05.30 -14:05:23.9
11:38:13.89 -14:16:00.1
11:36:13.42 -12:48:11.3
11:21:22.79 -08:24:18.5
11:37:24.43 -13:21:01.6
###################################################################################
11:36:39.89 -13:59:09.0 -- not an asteroid (will add it to exclusion list)
11:34:03.19 -14:39:25.4 -- not an asteroid (will add it to exclusion list)
11:38:08.65 -13:11:34.4 -- not an asteroid (will add it to exclusion list)
11:37:41.87 -14:09:45.7 -- not an asteroid (will add it to exclusion list)
11:34:43.37 -15:05:19.8 -- not an asteroid (will add it to exclusion list)
11:37:46.95 -12:56:26.8 -- not an asteroid (will add it to exclusion list)
11:38:18.25 -14:28:37.6 -- not an asteroid (will add it to exclusion list)
11:37:23.51 -13:21:01.0 -- not an asteroid (will add it to exclusion list)
11:33:30.59 -14:56:53.1 -- not an asteroid (will add it to exclusion list)
11:39:08.01 -07:58:29.6 -- not an asteroid (will add it to exclusion list)
11:36:32.91 -13:06:04.1 -- not an asteroid (will add it to exclusion list)
11:34:09.42 -14:37:18.7 -- not an asteroid (will add it to exclusion list)
11:39:03.40 -11:05:30.6 -- not an asteroid (will add it to exclusion list)
11:34:47.71 -13:39:26.4 -- not an asteroid (will add it to exclusion list)
11:37:30.09 -13:39:15.0 -- not an asteroid (will add it to exclusion list)
11:37:03.22 -12:47:30.8 -- not an asteroid (will add it to exclusion list)
11:35:17.13 -13:22:17.1 -- not an asteroid (will add it to exclusion list)
11:35:48.36 -11:52:40.0 -- not an asteroid (will add it to exclusion list)
11:36:30.21 -13:18:27.1 -- not an asteroid (will add it to exclusion list)
11:34:10.48 -14:03:32.8 -- not an asteroid (will add it to exclusion list)
11:37:26.61 -12:15:01.0 -- not an asteroid (will add it to exclusion list)
11:39:46.72 -09:32:41.4 -- not an asteroid (will add it to exclusion list)
11:39:14.87 -10:20:03.3 -- not an asteroid (will add it to exclusion list)
11:34:11.29 -13:58:17.1 -- not an asteroid (will add it to exclusion list)
11:37:26.61 -12:03:55.0 -- not an asteroid (will add it to exclusion list)
11:39:18.26 -10:06:52.4 -- not an asteroid (will add it to exclusion list)
11:35:18.51 -13:48:53.1 -- not an asteroid (will add it to exclusion list)
11:36:50.82 -14:10:28.1 -- not an asteroid (will add it to exclusion list)
11:35:22.14 -14:40:20.0 -- not an asteroid (will add it to exclusion list)
11:37:23.57 -15:07:57.6 -- not an asteroid (will add it to exclusion list)
11:36:55.49 -14:39:31.2 -- not an asteroid (will add it to exclusion list)
11:37:05.54 -14:18:14.3 -- not an asteroid (will add it to exclusion list)
11:35:58.25 -14:33:22.8 -- not an asteroid (will add it to exclusion list)
11:39:28.39 -11:04:18.7 -- not an asteroid (will add it to exclusion list)
11:33:27.53 -14:58:19.7 -- not an asteroid (will add it to exclusion list)
11:34:41.51 -14:51:05.4 -- not an asteroid (will add it to exclusion list)
11:35:55.34 -13:57:47.5 -- not an asteroid (will add it to exclusion list)
11:38:32.66 -13:50:57.9 -- not an asteroid (will add it to exclusion list)
11:38:32.15 -13:33:11.6 -- not an asteroid (will add it to exclusion list)
11:35:52.16 -15:04:16.9 -- not an asteroid (will add it to exclusion list)
11:34:03.46 -15:02:33.4 -- not an asteroid (will add it to exclusion list)
11:34:48.16 -14:11:39.7 -- not an asteroid (will add it to exclusion list)
11:37:29.78 -14:06:12.4 -- not an asteroid (will add it to exclusion list)
11:38:40.13 -13:56:04.8 -- not an asteroid (will add it to exclusion list)
11:34:14.83 -14:57:18.6 -- not an asteroid (will add it to exclusion list)
11:38:41.31 -11:50:51.6 -- not an asteroid (will add it to exclusion list)
11:34:58.99 -14:40:08.0 -- not an asteroid (will add it to exclusion list)
11:38:24.32 -14:43:02.6 -- not an asteroid (will add it to exclusion list)
11:33:52.12 -14:36:01.0 -- not an asteroid (will add it to exclusion list)
11:38:32.23 -11:26:48.1 -- not an asteroid (will add it to exclusion list)
11:37:55.43 -14:08:05.2 -- not an asteroid (will add it to exclusion list)
11:38:48.95 -13:54:40.7 -- not an asteroid (will add it to exclusion list)
11:23:34.80 -06:19:03.5 -- asteroid (will NOT add it to exclusion list)
11:38:49.17 -12:52:41.1 -- not an asteroid (will add it to exclusion list)
11:36:33.63 -14:17:46.3 -- not an asteroid (will add it to exclusion list)
11:37:05.30 -14:05:23.9 -- not an asteroid (will add it to exclusion list)
11:38:13.89 -14:16:00.1 -- not an asteroid (will add it to exclusion list)
11:36:13.42 -12:48:11.3 -- not an asteroid (will add it to exclusion list)
11:21:22.79 -08:24:18.5 -- asteroid (will NOT add it to exclusion list)
11:37:24.43 -13:21:01.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
11:33:27.53 -14:58:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:33:30.59 -14:56:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:33:52.12 -14:36:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:03.19 -14:39:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:03.46 -15:02:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:09.42 -14:37:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:10.48 -14:03:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:11.29 -13:58:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:14.83 -14:57:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:41.51 -14:51:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:43.37 -15:05:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:47.71 -13:39:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:48.16 -14:11:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:58.99 -14:40:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:17.13 -13:22:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:18.51 -13:48:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:22.14 -14:40:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:48.36 -11:52:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:52.16 -15:04:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:55.34 -13:57:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:58.25 -14:33:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:13.42 -12:48:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:30.21 -13:18:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:32.91 -13:06:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:33.63 -14:17:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:39.89 -13:59:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:50.82 -14:10:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:36:55.49 -14:39:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:03.22 -12:47:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:05.30 -14:05:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:05.54 -14:18:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:23.51 -13:21:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:23.57 -15:07:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:24.43 -13:21:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:26.61 -12:03:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:26.61 -12:15:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:29.78 -14:06:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:30.09 -13:39:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:41.87 -14:09:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:46.95 -12:56:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:37:55.43 -14:08:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:08.65 -13:11:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:13.89 -14:16:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:18.25 -14:28:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:24.32 -14:43:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:32.15 -13:33:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:32.23 -11:26:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:32.66 -13:50:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:40.13 -13:56:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:41.31 -11:50:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:48.95 -13:54:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:38:49.17 -12:52:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:39:03.40 -11:05:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:39:08.01 -07:58:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:39:14.87 -10:20:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:39:18.26 -10:06:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:39:28.39 -11:04:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:39:46.72 -09:32:41.4 -- 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)
11:33:27.53 -14:58:19.7 -- not a known variable star
11:33:30.59 -14:56:53.1 -- not a known variable star
11:33:52.12 -14:36:01.0 -- not a known variable star
11:34:03.19 -14:39:25.4 -- not a known variable star
11:34:03.46 -15:02:33.4 -- not a known variable star
11:34:09.42 -14:37:18.7 -- not a known variable star
11:34:10.48 -14:03:32.8 -- not a known variable star
11:34:11.29 -13:58:17.1 -- not a known variable star
11:34:14.83 -14:57:18.6 -- not a known variable star
11:34:41.51 -14:51:05.4 -- not a known variable star
11:34:43.37 -15:05:19.8 -- not a known variable star
11:34:47.71 -13:39:26.4 -- not a known variable star
11:34:48.16 -14:11:39.7 -- not a known variable star
11:34:58.99 -14:40:08.0 -- not a known variable star
11:35:17.13 -13:22:17.1 -- not a known variable star
11:35:18.51 -13:48:53.1 -- not a known variable star
11:35:22.14 -14:40:20.0 -- not a known variable star
11:35:48.36 -11:52:40.0 -- not a known variable star
11:35:52.16 -15:04:16.9 -- not a known variable star
11:35:55.34 -13:57:47.5 -- not a known variable star
11:35:58.25 -14:33:22.8 -- not a known variable star
11:36:13.42 -12:48:11.3 -- not a known variable star
11:36:30.21 -13:18:27.1 -- not a known variable star
11:36:32.91 -13:06:04.1 -- not a known variable star
11:36:33.63 -14:17:46.3 -- not a known variable star
11:36:39.89 -13:59:09.0 -- not a known variable star
11:36:50.82 -14:10:28.1 -- not a known variable star
11:36:55.49 -14:39:31.2 -- not a known variable star
11:37:03.22 -12:47:30.8 -- not a known variable star
11:37:05.30 -14:05:23.9 -- not a known variable star
11:37:05.54 -14:18:14.3 -- not a known variable star
11:37:23.51 -13:21:01.0 -- not a known variable star
11:37:23.57 -15:07:57.6 -- not a known variable star
11:37:24.43 -13:21:01.6 -- not a known variable star
11:37:26.61 -12:03:55.0 -- not a known variable star
11:37:26.61 -12:15:01.0 -- not a known variable star
11:37:29.78 -14:06:12.4 -- not a known variable star
11:37:30.09 -13:39:15.0 -- not a known variable star
11:37:41.87 -14:09:45.7 -- not a known variable star
11:37:46.95 -12:56:26.8 -- not a known variable star
11:37:55.43 -14:08:05.2 -- not a known variable star
11:38:08.65 -13:11:34.4 -- not a known variable star
11:38:13.89 -14:16:00.1 -- not a known variable star
11:38:18.25 -14:28:37.6 -- not a known variable star
11:38:24.32 -14:43:02.6 -- not a known variable star
11:38:32.15 -13:33:11.6 -- not a known variable star
11:38:32.23 -11:26:48.1 -- not a known variable star
11:38:32.66 -13:50:57.9 -- not a known variable star
11:38:40.13 -13:56:04.8 -- not a known variable star
11:38:41.31 -11:50:51.6 -- not a known variable star
11:38:48.95 -13:54:40.7 -- not a known variable star
11:38:49.17 -12:52:41.1 -- not a known variable star
11:39:03.40 -11:05:30.6 -- not a known variable star
11:39:08.01 -07:58:29.6 -- not a known variable star
11:39:14.87 -10:20:03.3 -- not a known variable star
11:39:18.26 -10:06:52.4 -- not a known variable star
11:39:28.39 -11:04:18.7 -- not a known variable star
11:39:46.72 -09:32:41.4 -- not a known variable star
Found 58 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
58 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
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461093.75036052 -observatory 500
23:23:35.96 -01:56:26.5 Mercury (-0.1mag)
23:04:50.82 -07:27:24.1 Venus (-3.9mag)
21:43:03.97 -14:51:33.8 Mars (1.1mag)
07:06:04.85 +22:54:22.2 Jupiter (-2.5mag)
00:05:28.27 -01:44:14.1 Saturn (1.0mag)
03:39:59.82 +19:21:44.9 Uranus (5.7mag)
00:03:41.52 -01:01:33.2 Neptune (7.8mag)
20:29:07.66 -22:59:32.7 Pluto (14.5mag)
01:58:41.37 +16:43:00.1 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 22 00:58 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461093.75036052:
07:06:11.19 +22:54:11.8 Io (5.4mag)
07:06:17.50 +22:53:58.3 Europa (5.5mag)
07:05:57.44 +22:54:44.6 Ganymede (4.9mag)
07:06:25.13 +22:53:54.2 Callisto (6.2mag)
07:09:14.20 +23:10:42.7 Himalia (15.0mag)
07:06:08.65 +22:54:15.9 Thebe (15.9mag)
07:08:39.21 +23:19:14.5 Elara (17.0mag)
07:01:38.67 +24:02:17.7 Pasiphae (17.0mag)
07:15:05.73 +22:42:23.8 Carme (18.1mag)
00:05:40.05 -01:44:18.4 Titan (8.8mag)
00:05:33.92 -01:44:12.4 Rhea (10.1mag)
00:05:23.89 -01:45:34.5 Iapetus (11.5mag)
00:05:29.45 -01:44:17.5 Hyperion (14.8mag)
00:07:32.53 -01:31:14.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 22 00:58 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.75036052:
08:46:31.69 +24:30:47.9 JWST
13:22:12.21 +54:04:45.2 Chandra
16:27:52.58 -52:19:12.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 22 00:58 spacecraft.txt
############################################################
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)2461093.75036052 at 500
16:59:52.75 -11:03:53.7 17.5mag 10P/Tempel 2
03:37:24.30 +28:58:09.3 18.0mag 123P/West-Hartley
08:23:29.73 +60:41:09.4 18.4mag 124P/Mrkos
21:19:53.67 -07:37:11.0 22.1mag 141P/Machholz
01:21:21.70 +11:56:28.3 17.7mag 145P/Shoemaker-Levy 5
11:02:53.55 +30:35:11.0 17.9mag 164P/Christensen
09:33:04.76 -33:51:32.9 18.0mag 195P/Hill
15:52:02.62 -06:35:20.2 19.2mag 210P/Christensen
18:17:18.18 -21:28:10.6 17.3mag 218P/LINEAR
16:21:43.91 -18:10:48.0 15.2mag 235P/LINEAR
03:56:31.58 +27:45:33.9 17.8mag 240P/NEAT
15:17:44.60 +06:37:59.3 14.8mag 24P/Schaumasse
11:23:28.75 -03:23:00.7 17.4mag 29P/Schwassmann-Wachmann 1
07:03:47.15 +27:24:51.9 19.6mag 407P/PanSTARRS-Fuls
17:07:18.29 -11:19:11.6 17.6mag 40P/Vaisala 1
11:02:09.12 -08:51:33.4 16.6mag 43P/Wolf-Harrington
13:25:30.08 -05:49:57.5 20.0mag 489P/Denning
04:34:26.43 +48:34:05.7 17.8mag 493P/2024 Q2 (LONEOS)
06:04:25.47 +47:30:23.4 17.7mag 63P/Wild 1
23:14:48.00 -02:06:27.3 16.2mag 78P/Gehrels 2
20:01:51.91 -22:17:27.5 14.9mag 88P/Howell
15:27:57.55 -29:01:08.5 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.68 -72:35:34.3 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:49.14 +31:12:55.1 18.2mag C/2017 K2 (PanSTARRS)
20:06:41.47 -65:11:49.0 18.1mag C/2020 V2 (ZTF)
17:21:42.86 +04:21:59.5 16.3mag C/2021 G2 (ATLAS)
03:35:45.66 +24:36:49.3 15.8mag C/2022 N2 (PanSTARRS)
09:08:11.24 +29:50:02.8 15.3mag C/2022 QE78 (ATLAS)
08:35:38.79 -06:33:04.0 16.7mag C/2022 R6 (PanSTARRS)
23:53:09.49 +48:26:59.8 18.0mag C/2023 C2 (ATLAS)
09:51:01.40 -20:45:08.2 17.5mag C/2023 F3 (ATLAS)
20:34:56.96 +61:14:31.3 17.3mag C/2023 H5 (Lemmon)
19:34:30.81 -03:24:18.8 16.1mag C/2023 R1 (PANSTARRS)
02:48:57.27 +35:40:31.5 18.5mag C/2023 RS61 (PanSTARRS)
21:01:36.85 +81:20:04.0 18.0mag C/2023 X2 (Lemmon)
06:39:01.26 +63:49:21.5 17.3mag C/2024 A1 (ATLAS)
01:57:28.24 -24:29:47.1 11.2mag C/2024 E1 (Wierzchos)
11:44:54.07 -02:33:44.5 18.1mag C/2024 G2 (ATLAS)
19:28:24.61 +00:39:24.5 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.55 -01:42:07.0 17.7mag C/2024 G6 (ATLAS)
19:53:31.63 +03:16:11.4 15.6mag C/2024 J3 (ATLAS)
02:47:17.72 -31:33:22.2 15.4mag C/2024 T5 (ATLAS)
16:24:50.03 -58:16:05.0 15.6mag C/2025 A6 (Lemmon)
04:50:28.36 +62:12:11.5 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)
15:56:39.36 -12:56:24.2 14.8mag C/2025 L1 (ATLAS)
02:20:19.08 -19:06:47.6 16.7mag C/2025 Q3 (ATLAS)
02:09:42.00 +17:17:17.6 21.2mag C/2025 R2 (SWAN)
22:20:47.98 +17:39:23.2 16.4mag C/2025 R3 (PANSTARRS)
21:46:07.48 -16:51:40.0 21.5mag C/2025 T1 (ATLAS)
03:06:00.99 -20:31:10.9 18.3mag C/2026 A1 (MAPS)
21:03:23.96 +20:58:17.1 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 22 01:00 comets.txt
############################################################
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 00:58 asassn_transients_list.txt
############################################################
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 00:58 tocp_transients_list.txt